J/ApJS/258/11ivo://CDS.VizieR/J/ApJS/258/11doi:10.26093/cds/vizier.22580011CDSWeaver J.R.Kauffmann O.B.Ilbert O.Mccracken H.J.Moneti A.Toft S.,Brammer G.Shuntov M.Davidzon I.Hsieh B.C.Laigle C.Anastasiou A.,Jespersen C.K.Vinther J.Capak P.Casey C.M.Mcpartland C.J.R.,Milvang-Jensen B.Mobasher B.Sanders D.B.Zalesky L.Arnouts S.,Aussel H.Dunlop J.S.Faisst A.Franx M.Furtak L.J.Fynbo J.P.U.,Gould K.M.L.Greve T.R.Gwyn S.Kartaltepe J.S.Kashino D.,Koekemoer A.M.Kokorev V.Le Fevre O.Lilly S.Masters D.Magdis G.,Mehta V.Peng Y.Riechers D.A.Salvato M.Sawicki M.Scarlata C.,Scoville N.Shirley R.Silverman J.D.Sneppen A.Smolcic V.,Steinhardt C.Stern D.Tanaka M.Taniguchi Y.Teplitz H.I.Vaccari M.,Wang W.-H.Zamorani G.2023-03-29T19:43:55Z2022-07-04T08:45:12ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frgalaxiescatalogsinfrared-photometryvisible-astronomybroad-band-photometryultraviolet-photometryradio-sourcesx-ray-sourcesastronomical-object-identificationredshiftedstellar-massesThe Cosmic Evolution Survey (COSMOS) has become a cornerstone of extragalactic astronomy. Since the last public catalog in 2015, a wealth of new imaging and spectroscopic data have been collected in the COSMOS field. This paper describes the collection, processing, and analysis of these new imaging data to produce a new reference photometric redshift catalog. Source detection and multiwavelength photometry are performed for 1.7 million sources across the 2 deg^2^ of the COSMOS field, ~966000 of which are measured with all available broadband data using both traditional aperture photometric methods and a new profile-fitting photometric extraction tool, THE FARMER, which we have developed. A detailed comparison of the two resulting photometric catalogs is presented. Photometric redshifts are computed for all sources in each catalog utilizing two independent photometric redshift codes. Finally, a comparison is made between the performance of the photometric methodologies and of the redshift codes to demonstrate an exceptional degree of self-consistency in the resulting photometric redshifts. The i<21 sources have subpercent photometric redshift accuracy and even the faintest sources at 25<i<27 reach a precision of 5%. Finally, these results are discussed in the context of previous, current, and future surveys in the COSMOS field. Compared to COSMOS2015, it reaches the same photometric redshift precision at almost one magnitude deeper. Both photometric catalogs and their photometric redshift solutions and physical parameters will be made available through the usual astronomical archive systems (ESO Phase 3, IPAC-IRSA, and CDS).2022ApJS..258...11Whttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/258/11CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/ApJS/224/24 : The COSMOS2015 catalog (Laigle+, 2016)II/284 : COSMOS Multi-Wavelength Photometry Catalog (Capak+, 2007)J/ApJ/819/62 : The COSMOS-Legacy Survey (CLS) catalog (Civano+, 2016)J/ApJ/817/34 : C-COSMOS Legacy sources multiwavelength cataloghttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/258/11https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/258/11http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/258/11https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/258/11https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/258/11http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/258/11GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJS/258/11/classic (COSMOS2020 Photometric catalogue "Classic" created using SExtractor and IRACLEAN (COSMOS2020\_CLASSIC\_R1\_v2.1\_p3.fits))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJS/258/11/classic?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJS/258/11/classic?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJS/258/11/classic?GETtext/xml+votable180.050000true151.008533571.398278250.005555555555555556Cone search capability for table J/ApJS/258/11/farmer (COSMOS2020 Photometric catalogue "Farmer" created using The Farmer / The Tractor (COSMOS2020\_FARMER\_R1\_v2.2\_p3.fits) updated version, 29/03/2023)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJS/258/11/farmer?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJS/258/11/farmer?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJS/258/11/farmer?GETtext/xml+votable180.050000true150.477638322.328963450.005555555555555556Cone search capability for table J/ApJS/258/11/list (Fits image and catalogues)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJS/258/11/list?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJS/258/11/list?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJS/258/11/list?GETtext/xml+votable180.050000true150.060782.292950.0055555555555555565/6814 6/27245 27247 27250 27333 27344-27345-3.4771685954054845e-18 4.139003408266671e-18https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJS/258/11?format=asciiX-rayUVOpticalInfraredRadiodefaultJ/ApJS/258/11/classicCOSMOS2020 Photometric catalogue "Classic" created using SExtractor and IRACLEAN (COSMOS2020\_CLASSIC\_R1\_v2.1\_p3.fits)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintFHSCr?=- HSC\_r AUTO flux density (HSC\_r\_FLUX_AUTO)uJyphot.flux.density;em.opt.RdoublenullableSCBmagIso?=- SC_B ISO AB magnitude (SC\_B\_MAG_ISO)magphot.mag;em.opt.BfloatnullableEZzp975?=- EAZY 97.5% percentile of photo-z (ez\_z975)src.redshift.phot;stat.maxdoublenullableClassicClassic catalogue ID (ID)meta.id;meta.mainintRAJ2000Right ascension (J2000) (ALPHA_J2000)degpos.eq.ra;meta.mainindexedDEJ2000Declination (J2000) (DELTA_J2000)degpos.eq.dec;meta.mainindexedCxyimageCovariance of position X/Y (ERRXY_IMAGE)pixel**2stat.covariance;pos.cartesianfloatradFlux? Radius enclosing 50% of total flux in PSF-homogenized Ks-band image (FLUX_RADIUS)pixphys.angSize;em.IR.KfloatnullableRadKron? Reduced pseudo-radius derived from the izYJHKs detection image (KRON_RADIUS)phys.angSize;arith.ratiodoublenullableFlagHSC[0/1] Flag indicating quality of HSC imaging (0: clean, 1: masked) (FLAG_HSC)meta.codeintFlagSUPCAM[0/1] Flag indicating quality of Suprime-Cam imaging (0: clean, 1 :masked) (FLAG_SUPCAM)meta.codeintFCFHTuap2?=- CFHT_u 2 arcsec diameter aperture flux density (CFHT\_u\_FLUX_APER2)uJyphot.flux.density;em.opt.Ufloatnullablee_FCFHTuap2?=- CFHT_u 2 arcsec diameter aperture flux density error (CFHT\_u\_FLUXERR_APER2)uJystat.error;phot.flux.density;em.opt.UfloatnullableFCFHTuap3?=- CFHT_u 3 arcsec diameter aperture flux density (CFHT\_u\_FLUX_APER3)uJyphot.flux.density;em.opt.UfloatnullableFCFHTu?=- CFHT_u AUTO flux density (CFHT\_u\_FLUX_AUTO)uJyphot.flux.density;em.opt.Udoublenullablee_FCFHTu?=- CFHT_u AUTO flux density error (CFHT\_u\_FLUXERR_AUTO)uJystat.error;phot.flux.density;em.opt.UfloatnullableCFHTumagap2?=- CFHT_u 2 arcsec diameter aperture AB magnitude (CFHT\_u\_MAG_APER2)magphot.mag;em.opt.Ufloatnullablee_CFHTumagap2?=- CFHT_u 2 arcsec diameter aperture AB magnitude error (CFHT\_u\_MAGERR_APER2)magstat.error;phot.mag;em.opt.UdoublenullableCFHTumagap3?=- CFHT_u 3 arcsec diameter aperture AB magnitude (CFHT\_u\_MAG_APER3)magphot.mag;em.opt.Ufloatnullablee_CFHTumagap3?=- CFHT_u 3 arcsec diameter aperture AB magnitude error (CFHT\_u\_MAGERR_APER3)magstat.error;phot.mag;em.opt.UdoublenullableCFHTumagAuto?=- CFHT_u AUTO AB magnitude (CFHT\_u\_MAG_AUTO)magphot.mag;em.opt.Ufloatnullablee_CFHTumagAuto?=- CFHT_u AUTO AB magnitude error (CFHT\_u\_MAGERR_AUTO)magstat.error;phot.mag;em.opt.UdoublenullableCFHTumagIso?=- CFHT_u ISO AB magnitude (CFHT\_u\_MAG_ISO)magphot.mag;em.opt.Ufloatnullablee_CFHTumagIso?=- CFHT_u ISO AB magnitude error (CFHT\_u\_MAGERR_ISO)magstat.error;phot.mag;em.opt.UdoublenullableCFHTuFlag?=- CFHT_u Source Extractor internal flags (CFHT\_u\_FLAGS)meta.code;phot;em.opt.UintnullableCFHTuFlagIso?=- CFHT_u flags: 4 means saturated pixel (s) in the isophotal area (CFHT\_u\_IMAFLAGS_ISO)meta.code;phot;em.opt.UintnullableE(B-V)Galactic reddening E(B-V) (EBV_MW) (1)phys.absorption.galfloatFCFHTustarap2?=- CFHT_ustar 2 arcsec diameter aperture flux density (CFHT\_ustar\_FLUX_APER2)uJyphot.flux.density;em.opt.Udoublenullablee_FCFHTustarap2?=- CFHT_ustar 2 arcsec diameter aperture flux density error (CFHT\_ustar\_FLUXERR_APER2)uJystat.error;phot.flux.density;em.opt.UfloatnullableFCFHTustarap3?=- CFHT_ustar 3 arcsec diameter aperture flux density (CFHT\_ustar\_FLUX_APER3)uJyphot.flux.density;em.opt.Udoublenullablee_FCFHTustarap3? CFHT_ustar 3 arcsec diameter aperture flux density error (CFHT_ustarap3)uJystat.error;phot.flux.density;em.opt.UfloatnullableFCFHTustar?=- CFHT_ustar AUTO flux density (CFHT\_ustar\_FLUX_AUTO)uJyphot.flux.density;em.opt.Udoublenullablee_FCFHTustar?=- CFHT_ustar AUTO flux density error (CFHT\_ustar\_FLUXERR_AUTO)uJystat.error;phot.flux.density;em.opt.UfloatnullableCFHTustarmagap2?=- CFHT_ustar 2 arcsec diameter aperture AB magnitude (CFHT\_ustar\_MAG_APER2)magphot.mag;em.opt.Ufloatnullablee_CFHTustarmagap2?=- CFHT_ustar 2 arcsec diameter aperture AB magnitude error (CFHT\_ustar\_MAGERR_APER2)magstat.error;phot.mag;em.opt.UdoublenullableCFHTustarmagap3?=- CFHT_ustar 3 arcsec diameter aperture AB magnitude (CFHT\_ustar\_MAG_APER3)magphot.mag;em.opt.Ufloatnullablee_CFHTustarmagap3?=- CFHT_ustar 3 arcsec diameter aperture AB magnitude error (CFHT\_ustar\_MAGERR_APER3)magstat.error;phot.mag;em.opt.UdoublenullableCFHTustarmagAuto?=- CFHT_ustar AUTO AB magnitude (CFHT\_ustar\_MAG_AUTO)magphot.mag;em.opt.Ufloatnullablee_CFHTustarmagAuto?=- CFHT_ustar AUTO AB magnitude error (CFHT\_ustar\_MAGERR_AUTO)magstat.error;phot.mag;em.opt.UdoublenullableCFHTustarmagIso?=- CFHT_ustar ISO AB magnitude (CFHT\_ustar\_MAG_ISO)magphot.mag;em.opt.Ufloatnullablee_CFHTustarmagIso?=- CFHT_ustar ISO AB magnitude error (CFHT\_ustar\_MAGERR_ISO)magstat.error;phot.mag;em.opt.UdoublenullableCFHTustarFlag?=- CFHT_ustar Source Extractor internal flags (CFHT\_ustar\_FLAGS)meta.code;phot;em.opt.UintnullableCFHTustarFlagIso?=- CFHT_ustar flags: 4 means saturated pixel (s) in the isophotal area (CFHT\_ustar\_IMAFLAGS_ISO)meta.code;phot;em.opt.UintnullableFHSCgap2?=- HSC\_g 2 arcsec diameter aperture flux density (HSC\_g\_FLUX_APER2)uJyphot.flux.density;em.opt.Bfloatnullablee_FHSCgap2?=- HSC\_g 2 arcsec diameter aperture flux density error (HSC\_g\_FLUXERR_APER2)uJystat.error;phot.flux.density;em.opt.BfloatnullableFHSCgap3?=- HSC\_g 3 arcsec diameter aperture flux density (HSC\_g\_FLUX_APER3)uJyphot.flux.density;em.opt.Bfloatnullablee_FHSCgap3?=- HSC\_g 3 arcsec diameter aperture flux density error (HSC\_gap3)uJystat.error;phot.flux.density;em.opt.BfloatnullableFHSCg?=- HSC\_g AUTO flux density (HSC\_g\_FLUX_AUTO)uJyphot.flux.density;em.opt.Bdoublenullablee_FHSCg?=- HSC\_g AUTO flux density error (HSC\_g\_FLUXERR_AUTO)uJystat.error;phot.flux.density;em.opt.BfloatnullableHSCgmagap2?=- HSC\_g 2 arcsec diameter aperture AB magnitude (HSC\_g\_MAG_APER2)magphot.mag;em.opt.Bfloatnullablee_HSCgmagap2?=- HSC\_g 2 arcsec diameter aperture AB magnitude error (HSC\_g\_MAGERR_APER2)magstat.error;phot.mag;em.opt.BdoublenullableHSCgmagap3?=- HSC\_g 3 arcsec diameter aperture AB magnitude (HSC\_g\_MAG_APER3)magphot.mag;em.opt.Bfloatnullablee_HSCgmagap3?=- HSC\_g 3 arcsec diameter aperture AB magnitude error (HSC\_g\_MAGERR_APER3)magstat.error;phot.mag;em.opt.BdoublenullableHSCgmagAuto?=- HSC\_g AUTO AB magnitude (HSC\_g\_MAG_AUTO)magphot.mag;em.opt.Bfloatnullablee_HSCgmagAuto?=- HSC\_g AUTO AB magnitude error (HSC\_g\_MAGERR_AUTO)magstat.error;phot.mag;em.opt.BdoublenullableHSCgmagIso?=- HSC\_g ISO AB magnitude (HSC\_g\_MAG_ISO)magphot.mag;em.opt.Bfloatnullablee_HSCgmagIso?=- HSC\_g ISO AB magnitude error (HSC\_g\_MAGERR_ISO)magstat.error;phot.mag;em.opt.BdoublenullableHSCgFlag?=- HSC\_g Source Extractor internal flags (HSC\_g\_FLAGS)meta.code;phot;em.opt.BintnullableHSCgFlagIso?=- HSC\_g flags: 4 means saturated pixel (s) in the isophotal area (HSC\_g\_IMAFLAGS_ISO)meta.code;phot;em.opt.BintnullableFHSCrap2?=- HSC\_r 2 arcsec diameter aperture flux density (HSC\_r\_FLUX_APER2)uJyphot.flux.density;em.opt.Rfloatnullablee_FHSCrap2?=- HSC\_r 2 arcsec diameter aperture flux density error (HSC\_r\_FLUXERR_APER2)uJystat.error;phot.flux.density;em.opt.RfloatnullableFHSCrap3?=- HSC\_r 3 arcsec diameter aperture flux density (HSC\_r\_FLUX_APER3)uJyphot.flux.density;em.opt.Rfloatnullablee_FHSCrap3?=- HSC\_r 3 arcsec diameter aperture flux density error (HSC\_rap3)uJystat.error;phot.flux.density;em.opt.Rfloatnullablee_FHSCr?=- HSC\_r AUTO flux density error (HSC\_r\_FLUXERR_AUTO)uJystat.error;phot.flux.density;em.opt.RfloatnullableHSCrmagap2?=- HSC\_r 2 arcsec diameter aperture AB magnitude (HSC\_r\_MAG_APER2)magphot.mag;em.opt.Rfloatnullablee_HSCrmagap2?=- HSC\_r 2 arcsec diameter aperture AB magnitude error (HSC\_r\_MAGERR_APER2)magstat.error;phot.mag;em.opt.RdoublenullableHSCrmagap3?=- HSC\_r 3 arcsec diameter aperture AB magnitude (HSC\_r\_MAG_APER3)magphot.mag;em.opt.Rfloatnullablee_HSCrmagap3?=- HSC\_r 3 arcsec diameter aperture AB magnitude error (HSC\_r\_MAGERR_APER3)magstat.error;phot.mag;em.opt.RdoublenullableHSCrmagAuto?=- HSC\_r AUTO AB magnitude (HSC\_r\_MAG_AUTO)magphot.mag;em.opt.Rfloatnullablee_HSCrmagAuto?=- HSC\_r AUTO AB magnitude error (HSC\_r\_MAGERR_AUTO)magstat.error;phot.mag;em.opt.RdoublenullableHSCrmagIso?=- HSC\_r ISO AB magnitude (HSC\_r\_MAG_ISO)magphot.mag;em.opt.Rfloatnullablee_HSCrmagIso?=- HSC\_r ISO AB magnitude error (HSC\_r\_MAGERR_ISO)magstat.error;phot.mag;em.opt.RdoublenullableHSCrFlag?=- HSC\_r Source Extractor internal flags (HSC\_r\_FLAGS)meta.code;phot;em.opt.RintnullableHSCrFlagIso?=- HSC\_r flags: 4 means saturated pixel (s) in the isophotal area (HSC\_r\_IMAFLAGS_ISO)meta.code;phot;em.opt.RintnullableFHSCiap2?=- HSC\_i 2 arcsec diameter aperture flux density (HSC\_i\_FLUX_APER2)uJyphot.flux.density;em.opt.Ifloatnullablee_FHSCiap2?=- HSC\_i 2 arcsec diameter aperture flux density error (HSC\_i\_FLUXERR_APER2)uJystat.error;phot.flux.density;em.opt.IfloatnullableFHSCiap3?=- HSC\_i 3 arcsec diameter aperture flux density (HSC\_i\_FLUX_APER3)uJyphot.flux.density;em.opt.Ifloatnullablee_FHSCiap3?=- HSC\_i 3 arcsec diameter aperture flux density error (HSC\_iap3)uJystat.error;phot.flux.density;em.opt.IfloatnullableFHSCi?=- HSC\_i AUTO flux density (HSC\_i\_FLUX_AUTO)uJyphot.flux.density;em.opt.Idoublenullablee_FHSCi?=- HSC\_i AUTO flux density error (HSC\_i\_FLUXERR_AUTO)uJystat.error;phot.flux.density;em.opt.IfloatnullableHSCimagap2?=- HSC\_i 2 arcsec diameter aperture AB magnitude (HSC\_i\_MAG_APER2)magphot.mag;em.opt.Ifloatnullablee_HSCimagap2?=- HSC\_i 2 arcsec diameter aperture AB magnitude error (HSC\_i\_MAGERR_APER2)magstat.error;phot.mag;em.opt.IdoublenullableHSCimagap3?=- HSC\_i 3 arcsec diameter aperture AB magnitude (HSC\_i\_MAG_APER3)magphot.mag;em.opt.Ifloatnullablee_HSCimagap3?=- HSC\_i 3 arcsec diameter aperture AB magnitude error (HSC\_i\_MAGERR_APER3)magstat.error;phot.mag;em.opt.IdoublenullableHSCimagAuto?=- HSC\_i AUTO AB magnitude (HSC\_i\_MAG_AUTO)magphot.mag;em.opt.Ifloatnullablee_HSCimagAuto?=- HSC\_i AUTO AB magnitude error (HSC\_i\_MAGERR_AUTO)magstat.error;phot.mag;em.opt.IdoublenullableHSCimagIso?=- HSC\_i ISO AB magnitude (HSC\_i\_MAG_ISO)magphot.mag;em.opt.Ifloatnullablee_HSCimagIso?=- HSC\_i ISO AB magnitude error (HSC\_i\_MAGERR_ISO)magstat.error;phot.mag;em.opt.IdoublenullableHSCiFlag?=- HSC\_i Source Extractor internal flags (HSC\_i\_FLAGS)meta.code;phot;em.opt.IintnullableHSCiFlagIso?=- HSC\_i flags: 4 means saturated pixel (s) in the isophotal area (HSC\_i\_IMAFLAGS_ISO)meta.code;phot;em.opt.IintnullableFHSCzap2?=- HSC_z 2 arcsec diameter aperture flux density (HSC\_z\_FLUX_APER2)uJyphot.flux.density;em.opt.Ifloatnullablee_FHSCzap2?=- HSC_z 2 arcsec diameter aperture flux density error (HSC\_z\_FLUXERR_APER2)uJystat.error;phot.flux.density;em.opt.IfloatnullableFHSCzap3?=- HSC_z 3 arcsec diameter aperture flux density (HSC\_z\_FLUX_APER3)uJyphot.flux.density;em.opt.Ifloatnullablee_FHSCzap3?=- HSC_z 3 arcsec diameter aperture flux density error (HSC\_zap3)uJystat.error;phot.flux.density;em.opt.IfloatnullableFHSCz?=- HSC_z AUTO flux density (HSC\_z\_FLUX_AUTO)uJyphot.flux.density;em.opt.Idoublenullablee_FHSCz?=- HSC\_z AUTO flux density error (HSC\_z\_FLUXERR_AUTO)uJystat.error;phot.flux.density;em.opt.IfloatnullableHSCzmagap2?=- HSC_z 2 arcsec diameter aperture AB magnitude (HSC\_z\_MAG_APER2)magphot.mag;em.opt.Ifloatnullablee_HSCzmagap2?=- HSC_z 2 arcsec diameter aperture AB magnitude error (HSC\_z\_MAGERR_APER2)magstat.error;phot.mag;em.opt.IdoublenullableHSCzmagap3?=- HSC_z 3 arcsec diameter aperture AB magnitude (HSC\_z\_MAG_APER3)magphot.mag;em.opt.Ifloatnullablee_HSCzmagap3?=- HSC_z 3 arcsec diameter aperture AB magnitude error (HSC\_z\_MAGERR_APER3)magstat.error;phot.mag;em.opt.IdoublenullableHSCzmagAuto?=- HSC_z AUTO AB magnitude (HSC\_z\_MAG_AUTO)magphot.mag;em.opt.Ifloatnullablee_HSCzmagAuto?=- HSC_z AUTO AB magnitude error (HSC\_z\_MAGERR_AUTO)magstat.error;phot.mag;em.opt.IdoublenullableHSCzmagIso?=- HSC\_z ISO AB magnitude (HSC\_z\_MAG_ISO)magphot.mag;em.opt.Ifloatnullablee_HSCzmagIso?=- HSC_z ISO AB magnitude error (HSC\_z\_MAGERR_ISO)magstat.error;phot.mag;em.opt.IdoublenullableHSCzFlag?=- HSC_z Source Extractor internal flags (HSC\_z\_FLAGS)meta.code;phot;em.opt.IintnullableHSCzFlagIso?=- HSC_z flags: 4 means saturated pixel (s) in the isophotal area (HSC\_z\_IMAFLAGS_ISO)meta.code;phot;em.opt.IintnullableFHSCyap2?=- HSC_y 2 arcsec diameter aperture flux density (HSC\_y\_FLUX_APER2)uJyphot.flux.density;em.opt.Ifloatnullablee_FHSCyap2?=- HSC_y 2 arcsec diameter aperture flux density error (HSC\_y\_FLUXERR_APER2)uJystat.error;phot.flux.density;em.opt.IfloatnullableFHSCyap3?=- HSC_y 3 arcsec diameter aperture flux density (HSC\_y\_FLUX_APER3)uJyphot.flux.density;em.opt.Ifloatnullablee_FHSCyap3?=- HSC_y 3 arcsec diameter aperture flux density error (HSC\_yap3)uJystat.error;phot.flux.density;em.opt.IfloatnullableFHSCy?=- HSC_y AUTO flux density (HSC\_y\_FLUX_AUTO)uJyphot.flux.density;em.opt.Idoublenullablee_FHSCy?=- HSC\_y AUTO flux density error (HSC\_y\_FLUXERR_AUTO)uJystat.error;phot.flux.density;em.opt.IfloatnullableHSCymagap2?=- HSC_y 2 arcsec diameter aperture AB magnitude (HSC\_y\_MAG_APER2)magphot.mag;em.opt.Ifloatnullablee_HSCymagap2?=- HSC_y 2 arcsec diameter aperture AB magnitude error (HSC\_y\_MAGERR_APER2)magstat.error;phot.mag;em.opt.IdoublenullableHSCymagap3?=- HSC_y 3 arcsec diameter aperture AB magnitude (HSC\_y\_MAG_APER3)magphot.mag;em.opt.Ifloatnullablee_HSCymagap3?=- HSC_y 3 arcsec diameter aperture AB magnitude error (HSC\_y\_MAGERR_APER3)magstat.error;phot.mag;em.opt.IdoublenullableHSCymagAuto?=- HSC_y AUTO AB magnitude (HSC\_y\_MAG_AUTO)magphot.mag;em.opt.Ifloatnullablee_HSCymagAuto?=- HSC_y AUTO AB magnitude error (HSC\_y\_MAGERR_AUTO)magstat.error;phot.mag;em.opt.IdoublenullableHSCymagIso?=- HSC_y ISO AB magnitude (HSC\_y\_MAG_ISO)magphot.mag;em.opt.Ifloatnullablee_HSCymagIso?=- HSC_y ISO AB magnitude error (HSC\_y\_MAGERR_ISO)magstat.error;phot.mag;em.opt.IdoublenullableHSCyFlag?=- HSC_y Source Extractor internal flags (HSC\_y\_FLAGS)meta.code;phot;em.opt.IintnullableHSCyFlagIso?=- HSC_y flags: 4 means saturated pixel (s) in the isophotal area (HSC\_y\_IMAFLAGS_ISO)meta.code;phot;em.opt.IintnullableFUVISTAYap2?=- UVISTA_Y 2 arcsec diameter aperture flux density (UVISTA\_Y\_FLUX_APER2)uJyphot.flux.density;em.IR.Jdoublenullablee_FUVISTAYap2?=- UVISTA_Y 2 arcsec diameter aperture flux density error (UVISTA_Y\_FLUXERR_APER2)uJystat.error;phot.flux.density;em.IR.JfloatnullableFUVISTAYap3?=- UVISTA_Y 3 arcsec diameter aperture flux density (UVISTA\_Y\_FLUX_APER3)uJyphot.flux.density;em.IR.Jdoublenullablee_FUVISTAYap3?=- UVISTA_Y 3 arcsec diameter aperture flux density error (UVISTA\_Yap3)uJystat.error;phot.flux.density;em.IR.JfloatnullableFUVISTAY?=- UVISTA_Y AUTO flux density (UVISTA\_Y\_FLUX_AUTO)uJyphot.flux.density;em.IR.Jdoublenullablee_FUVISTAY?=- UVISTA_Y AUTO flux density error (UVISTA\_Y\_FLUXERR_AUTO)uJystat.error;phot.flux.density;em.IR.JfloatnullableUVISTAYmagap2?=- UVISTA_Y 2 arcsec diameter aperture AB magnitude (UVISTA\_Y\_MAG_APER2)magphot.mag;em.IR.Jfloatnullablee_UVISTAYmagap2?=- UVISTA_Y 2 arcsec diameter aperture AB magnitude error (UVISTA\_Y\_MAGERR_APER2)magstat.error;phot.mag;em.IR.JdoublenullableUVISTAYmagap3?=- UVISTA_Y 3 arcsec diameter aperture AB magnitude (UVISTA\_Y\_MAG_APER3)magphot.mag;em.IR.Jfloatnullablee_UVISTAYmagap3?=- UVISTA_Y 3 arcsec diameter aperture AB magnitude error (UVISTA\_Y\_MAGERR_APER3)magstat.error;phot.mag;em.IR.JdoublenullableUVISTAYmagAuto?=- UVISTA_Y AUTO AB magnitude (UVISTA\_Y\_MAG_AUTO)magphot.mag;em.IR.Jfloatnullablee_UVISTAYmagAuto?=- UVISTA_Y AUTO AB magnitude error (UVISTA\_Y\_MAGERR_AUTO)magstat.error;phot.mag;em.IR.JdoublenullableUVISTAYmagIso?=- UVISTA_Y ISO AB magnitude (UVISTA\_Y\_MAG_ISO)magphot.mag;em.IR.Jfloatnullablee_UVISTAYmagIso?=- UVISTA_Y ISO AB magnitude error (UVISTA\_Y\_MAGERR_ISO)magstat.error;phot.mag;em.IR.JdoublenullableUVISTAYFlag?=- UVISTA_Y Source Extractor internal flags (UVISTA\_Y\_FLAGS)meta.code;phot;em.IR.JintnullableUVISTAYFlagIso?=- UVISTA_Y flags: 4 means saturated pixel (s) in the isophotal area (UVISTA\_Y\_IMAFLAGS_ISO)meta.code;phot;em.IR.JintnullableFUVISTAJap2?=- UVISTA_J 2 arcsec diameter aperture flux density (UVISTA\_J\_FLUX_APER2)uJyphot.flux.density;em.IR.Jdoublenullablee_FUVISTAJap2?=- UVISTA_J 2 arcsec diameter aperture flux density error (UVISTA\_J\_FLUXERR_APER2)uJystat.error;phot.flux.density;em.IR.JfloatnullableFUVISTAJap3?=- UVISTA_J 3 arcsec diameter aperture flux density (UVISTA\_J\_FLUX_APER3)uJyphot.flux.density;em.IR.Jdoublenullablee_FUVISTAJap3?=- UVISTA_J 3 arcsec diameter aperture flux density error (UVISTA\_Jap3)uJystat.error;phot.flux.density;em.IR.JfloatnullableFUVISTAJ?=- UVISTA_J AUTO flux density (UVISTA\_J\_FLUX_AUTO)uJyphot.flux.density;em.IR.Jdoublenullablee_FUVISTAJ?=- UVISTA_J AUTO flux density error (UVISTA\_J\_FLUXERR_AUTO)uJystat.error;phot.flux.density;em.IR.JfloatnullableUVISTAJmagap2?=- UVISTA_J 2 arcsec diameter aperture AB magnitude (UVISTA\_J\_MAG_APER2)magphot.mag;em.IR.JfloatnullableEZzphot?=- EAZY maximum a-posteriori photo-z (ez\_z\_phot)src.redshift.photdoublenullablee_UVISTAJmagap2?=- UVISTA_J 2 arcsec diameter aperture AB magnitude error (UVISTA\_J\_MAGERR_APER2)magstat.error;phot.mag;em.IR.JdoublenullableUVISTAJmagap3?=- UVISTA_J 3 arcsec diameter aperture AB magnitude (UVISTA\_J\_MAG_APER3)magphot.mag;em.IR.Jfloatnullablee_UVISTAJmagap3?=- UVISTA_J 3 arcsec diameter aperture AB magnitude error (UVISTA\_J\_MAGERR_APER3)magstat.error;phot.mag;em.IR.JdoublenullableUVISTAJmagAuto?=- UVISTA_J AUTO AB magnitude (UVISTA\_J\_MAG_AUTO)magphot.mag;em.IR.Jfloatnullablee_UVISTAJmagAuto?=- UVISTA_J AUTO AB magnitude error (UVISTA\_J\_MAGERR_AUTO)magstat.error;phot.mag;em.IR.JdoublenullableUVISTAJmagIso?=- UVISTA_J ISO AB magnitude (UVISTA\_J\_MAG_ISO)magphot.mag;em.IR.Jfloatnullablee_UVISTAJmagIso?=- UVISTA_J ISO AB magnitude error (UVISTA\_J\_MAGERR_ISO)magstat.error;phot.mag;em.IR.JdoublenullableUVISTAJFlag?=- UVISTA_J Source Extractor internal flags (UVISTA\_J\_FLAGS)meta.code;phot;em.IR.JintnullableUVISTAJFlagIso?=- UVISTA_J flags: 4 means saturated pixel (s) in the isophotal area (UVISTA\_J\_IMAFLAGS_ISO)meta.code;phot;em.IR.JintnullableFUVISTAHap2?=- UVISTA_H 2 arcsec diameter aperture flux density (UVISTA\_H\_FLUX_APER2)uJyphot.flux.density;em.IR.Hdoublenullablee_FUVISTAHap2?=- UVISTA_H 2 arcsec diameter aperture flux density error (UVISTA\_H\_FLUXERR_APER2)uJystat.error;phot.flux.density;em.IR.HfloatnullableFUVISTAHap3?=- UVISTA_H 3 arcsec diameter aperture flux density (UVISTA\_H\_FLUX_APER3)uJyphot.flux.density;em.IR.Hdoublenullablee_FUVISTAHap3?=- UVISTA_H 3 arcsec diameter aperture flux density error (UVISTA\_Hap3)uJystat.error;phot.flux.density;em.IR.HfloatnullableFUVISTAH?=- UVISTA_H AUTO flux density (UVISTA\_H\_FLUX_AUTO)uJyphot.flux.density;em.IR.Hdoublenullablee_FUVISTAH?=- UVISTA\_H AUTO flux density error (UVISTA\_H\_FLUXERR_AUTO)uJystat.error;phot.flux.density;em.IR.HfloatnullableUVISTAHmagap2?=- UVISTA_H 2 arcsec diameter aperture AB magnitude (UVISTA\_H\_MAG_APER2)magphot.mag;em.IR.Hfloatnullablee_UVISTAHmagap2?=- UVISTA_H 2 arcsec diameter aperture AB magnitude error (UVISTA\_H\_MAGERR_APER2)magstat.error;phot.mag;em.IR.HdoublenullableUVISTAHmagap3?=- UVISTA_H 3 arcsec diameter aperture AB magnitude (UVISTA\_H\_MAG_APER3)magphot.mag;em.IR.Hfloatnullablee_UVISTAHmagap3?=- UVISTA_H 3 arcsec diameter aperture AB magnitude error (UVISTA\_H\_MAGERR_APER3)magstat.error;phot.mag;em.IR.HdoublenullableUVISTAHmagAuto?=- UVISTA_H AUTO AB magnitude (UVISTA\_H\_MAG_AUTO)magphot.mag;em.IR.Hfloatnullablee_UVISTAHmagAuto?=- UVISTA_H AUTO AB magnitude error (UVISTA\_H\_MAGERR_AUTO)magstat.error;phot.mag;em.IR.HdoublenullableUVISTAHmagIso?=- UVISTA_H ISO AB magnitude (UVISTA\_H\_MAG_ISO)magphot.mag;em.IR.Hfloatnullablee_UVISTAHmagIso?=- UVISTA_H ISO AB magnitude error (UVISTA\_H\_MAGERR_ISO)magstat.error;phot.mag;em.IR.HdoublenullableUVISTAHFlag?=- UVISTA_H Source Extractor internal flags (UVISTA\_H\_FLAGS)meta.code;phot;em.IR.HintnullableUVISTAHFlagIso?=- UVISTA_H flags: 4 means saturated pixel (s) in the isophotal area (UVISTA\_H\_IMAFLAGS_ISO)meta.code;phot;em.IR.HintnullableFUVISTAKsap2?=- UVISTA_Ks 2 arcsec diameter aperture flux density (UVISTA\_Ks\_FLUX_APER2)uJyphot.flux.density;em.IR.Kdoublenullablee_FUVISTAKsap2?=- UVISTA_Ks 2 arcsec diameter aperture flux density error (UVISTA\_Ks\_FLUXERR_APER2)uJystat.error;phot.flux.density;em.IR.KfloatnullableFUVISTAKsap3?=- UVISTA_Ks 3 arcsec diameter aperture flux density (UVISTA\_Ks\_FLUX_APER3)uJyphot.flux.density;em.IR.Kdoublenullablee_FUVISTAKsap3?=- UVISTA_Ks 3 arcsec diameter aperture flux density error (UVISTA\_Ksap3)uJystat.error;phot.flux.density;em.IR.KfloatnullableFUVISTAKs?=- UVISTA_Ks AUTO flux density (UVISTA\_Ks\_FLUX_AUTO)uJyphot.flux.density;em.IR.Kdoublenullablee_FUVISTAKs?=- UVISTA_Ks AUTO flux density error (UVISTA\_Ks\_FLUXERR_AUTO)uJystat.error;phot.flux.density;em.IR.KfloatnullableUVISTAKsmagap2?=- UVISTA_Ks 2 arcsec diameter aperture AB magnitude (UVISTA\_Ks\_MAG_APER2)magphot.mag;em.IR.Kfloatnullablee_UVISTAKsmagap2?=- UVISTA_Ks 2 arcsec diameter aperture AB magnitude error (UVISTA\_Ks\_MAGERR_APER2)magstat.error;phot.mag;em.IR.KdoublenullableUVISTAKsmagap3?=- UVISTA_Ks 3 arcsec diameter aperture AB magnitude (UVISTA\_Ks\_MAG_APER3)magphot.mag;em.IR.Kfloatnullablee_UVISTAKsmagap3?=- UVISTA_Ks 3 arcsec diameter aperture AB magnitude error (UVISTA\_Ks\_MAGERR_APER3)magstat.error;phot.mag;em.IR.KdoublenullableUVISTAKsmagAuto?=- UVISTA_Ks AUTO AB magnitude (UVISTA\_Ks\_MAG_AUTO)magphot.mag;em.IR.Kfloatnullablee_UVISTAKsmagAuto?=- UVISTA_Ks AUTO AB magnitude error (UVISTA\_Ks\_MAGERR_AUTO)magstat.error;phot.mag;em.IR.KdoublenullableUVISTAKsmagIso?=- UVISTA_Ks ISO AB magnitude (UVISTA\_Ks\_MAG_ISO)magphot.mag;em.IR.Kfloatnullablee_UVISTAKsmagIso?=- UVISTA_Ks ISO AB magnitude error (UVISTA\_Ks\_MAGERR_ISO)magstat.error;phot.mag;em.IR.KdoublenullableUVISTAKsFlag?=- UVISTA_Ks Source Extractor internal flags (UVISTA\_Ks\_FLAGS)meta.code;phot;em.IR.KintnullableUVISTAKsFlagIso?=- UVISTA_Ks flags: 4 means saturated pixel (s) in the isophotal area (UVISTA\_Ks\_IMAFLAGS_ISO)meta.code;phot;em.IR.KintnullableFSCIB427ap2?=- SC_IB427 2 arcsec diameter aperture flux density (SC\_IB427\_FLUX_APER2)uJyphot.flux.density;em.opt.Bfloatnullablee_FSCIB427ap2?=- SC_IB427 2 arcsec diameter aperture flux density error (SC\_IB427\_FLUXERR_APER2)uJystat.error;phot.flux.density;em.opt.BfloatnullableFSCIB427ap3?=- SC_IB427 3 arcsec diameter aperture flux density (SC\_IB427\_FLUX_APER3)uJyphot.flux.density;em.opt.Bfloatnullablee_FSCIB427ap3?=- SC_IB427 3 arcsec diameter aperture flux density error (SC\_IB427ap3)uJystat.error;phot.flux.density;em.opt.BfloatnullableFSCIB427?=- SC_IB427 AUTO flux density (SC\_IB427\_FLUX_AUTO)uJyphot.flux.density;em.opt.Bdoublenullablee_FSCIB427?=- SC_IB427 AUTO flux density error (SC\_IB427\_FLUXERR_AUTO)uJystat.error;phot.flux.density;em.opt.BfloatnullableSCIB427magap2?=- SC_IB427 2 arcsec diameter aperture AB magnitude (SC\_IB427\_MAG_APER2)magphot.mag;em.opt.Bfloatnullablee_SCIB427magap2?=- SC_IB427 2 arcsec diameter aperture AB magnitude error (SC\_IB427\_MAGERR_APER2)magstat.error;phot.mag;em.opt.BdoublenullableSCIB427magap3?=- SC_IB427 3 arcsec diameter aperture AB magnitude (SC\_IB427\_MAG_APER3)magphot.mag;em.opt.Bfloatnullablee_SCIB427magap3?=- SC_IB427 3 arcsec diameter aperture AB magnitude error (SC\_IB427\_MAGERR_APER3)magstat.error;phot.mag;em.opt.BdoublenullableSCIB427magAuto?=- SC_IB427 AUTO AB magnitude (SC\_IB427\_MAG_AUTO)magphot.mag;em.opt.Bfloatnullablee_SCIB427magAuto?=- SC_IB427 AUTO AB magnitude error (SC\_IB427\_MAGERR_AUTO)magstat.error;phot.mag;em.opt.BdoublenullableSCIB427magIso?=- SC_IB427 ISO AB magnitude (SC\_IB427\_MAG_ISO)magphot.mag;em.opt.Bfloatnullablee_SCIB427magIso?=- SC_IB427 ISO AB magnitude error (SC\_IB427\_MAGERR_ISO)magstat.error;phot.mag;em.opt.BdoublenullableSCIB427Flag?=- SC_IB427 Source Extractor internal flags (SC\_IB427\_FLAGS)meta.code;phot;em.opt.BintnullableSCIB427FlagIso?=- SC_IB427 flags: 4 means saturated pixel (s) in the isophotal area (SC_IB427\_IMAFLAGS_ISO)meta.code;phot;em.opt.BintnullableFSCIB464ap2?=- SC_IB464 2 arcsec diameter aperture flux density (SC\_IB464\_FLUX_APER2)uJyphot.flux.density;em.opt.Bfloatnullablee_FSCIB464ap2?=- SC_IB464 2 arcsec diameter aperture flux density error (SC\_IB464\_FLUXERR_APER2)uJystat.error;phot.flux.density;em.opt.BfloatnullableFSCIB464ap3?=- SC_IB464 3 arcsec diameter aperture flux density (SC\_IB464\_FLUX_APER3)uJyphot.flux.density;em.opt.Bfloatnullablee_FSCIB464ap3?=- SC_IB464 3 arcsec diameter aperture flux density error (SC\_IB464ap3)uJystat.error;phot.flux.density;em.opt.BfloatnullableFSCIB464?=- SC_IB464 AUTO flux density (SC\_IB464\_FLUX_AUTO)uJyphot.flux.density;em.opt.Bdoublenullablee_FSCIB464?=- SC_IB464 AUTO flux density error (SC\_IB464\_FLUXERR_AUTO)uJystat.error;phot.flux.density;em.opt.BfloatnullableSCIB464magap2?=- SC_IB464 2 arcsec diameter aperture AB magnitude (SC\_IB464\_MAG_APER2)magphot.mag;em.opt.Bfloatnullablee_SCIB464magap2?=- SC_IB464 2 arcsec diameter aperture AB magnitude error (SC\_IB464\_MAGERR_APER2)magstat.error;phot.mag;em.opt.BdoublenullableSCIB464magap3?=- SC_IB464 3 arcsec diameter aperture AB magnitude (SC\_IB464\_MAG_APER3)magphot.mag;em.opt.Bfloatnullablee_SCIB464magap3?=- SC_IB464 3 arcsec diameter aperture AB magnitude error (SC\_IB464\_MAGERR_APER3)magstat.error;phot.mag;em.opt.BdoublenullableSCIB464magAuto?=- SC_IB464 AUTO AB magnitude (SC\_IB464\_MAG_AUTO)magphot.mag;em.opt.Bfloatnullablee_SCIB464magAuto?=- SC_IB464 AUTO AB magnitude error (SC\_IB464\_MAGERR_AUTO)magstat.error;phot.mag;em.opt.BdoublenullableSCIB464magIso?=- SC_IB464 ISO AB magnitude (SC\_IB464\_MAG_ISO)magphot.mag;em.opt.Bfloatnullablee_SCIB464magIso?=- SC_IB464 ISO AB magnitude error (SC\_IB464\_MAGERR_ISO)magstat.error;phot.mag;em.opt.BdoublenullableSCIB464Flag?=- SC_IB464 Source Extractor internal flags (SC\_IB464\_FLAGS)meta.code;phot;em.opt.BintnullableSCIB464FlagIso?=- SC_IB464 flags: 4 means saturated pixel (s) in the isophotal area (SC\_IB464\_IMAFLAGS_ISO)meta.code;phot;em.opt.BintnullableFSCIA484ap2?=- SC_IA484 2 arcsec diameter aperture flux density (SC\_IA484\_FLUX_APER2)uJyphot.flux.density;em.opt.Bfloatnullablee_FSCIA484ap2?=- SC_IA484 2 arcsec diameter aperture flux density error (SC\_IA484\_FLUXERR_APER2)uJystat.error;phot.flux.density;em.opt.BfloatnullableFSCIA484ap3?=- SC_IA484 3 arcsec diameter aperture flux density (SC\_IA484\_FLUX_APER3)uJyphot.flux.density;em.opt.Bfloatnullablee_FSCIA484ap3?=- SC_IA484 3 arcsec diameter aperture flux density error (SC\_IA484ap3)uJystat.error;phot.flux.density;em.opt.BfloatnullableFSCIA484?=- SC_IA484 AUTO flux density (SC\_IA484\_FLUX_AUTO)uJyphot.flux.density;em.opt.Bdoublenullablee_FSCIA484?=- SC_IA484 AUTO flux density error (SC\_IA484\_FLUXERR_AUTO)uJystat.error;phot.flux.density;em.opt.BfloatnullableSCIA484magap2?=- SC_IA484 2 arcsec diameter aperture AB magnitude (SC\_IA484\_MAG_APER2)magphot.mag;em.opt.Bfloatnullablee_SCIA484magap2?=- SC_IA484 2 arcsec diameter aperture AB magnitude error (SC\_IA484\_MAGERR_APER2)magstat.error;phot.mag;em.opt.BdoublenullableSCIA484magap3?=- SC_IA484 3 arcsec diameter aperture AB magnitude (SC\_IA484\_MAG_APER3)magphot.mag;em.opt.Bfloatnullablee_SCIA484magap3?=- SC_IA484 3 arcsec diameter aperture AB magnitude error (SC\_IA484\_MAGERR_APER3)magstat.error;phot.mag;em.opt.BdoublenullableSCIA484magAuto?=- SC_IA484 AUTO AB magnitude (SC\_IA484\_MAG_AUTO)magphot.mag;em.opt.Bfloatnullablee_SCIA484magAuto?=- SC_IA484 AUTO AB magnitude error (SC\_IA484\_MAGERR_AUTO)magstat.error;phot.mag;em.opt.BdoublenullableSCIA484magIso?=- SC_IA484 ISO AB magnitude (SC\_IA484\_MAG_ISO)magphot.mag;em.opt.Bfloatnullablee_SCIA484magIso?=- SC_IA484 ISO AB magnitude error (SC\_IA484\_MAGERR_ISO)magstat.error;phot.mag;em.opt.BdoublenullableSCIA484Flag?=- SC_IA484 Source Extractor internal flags (SC\_IA484\_FLAGS)meta.code;phot;em.opt.BintnullableSCIA484FlagIso?=- SC_IA484 flags: 4 means saturated pixel (s) in the isophotal area (SC\_IA484\_IMAFLAGS_ISO)meta.code;phot;em.opt.BintnullableFSCIB505ap2?=- SC_IB505 2 arcsec diameter aperture flux density (SC\_IB505\_FLUX_APER2)uJyphot.flux.density;em.opt.Vfloatnullablee_FSCIB505ap2?=- SC_IB505 2 arcsec diameter aperture flux density error (SC\_IB505\_FLUXERR_APER2)uJystat.error;phot.flux.density;em.opt.VfloatnullableFSCIB505ap3?=- SC_IB505 3 arcsec diameter aperture flux density (SC\_IB505\_FLUX_APER3)uJyphot.flux.density;em.opt.Vfloatnullablee_FSCIB505ap3?=- SC_IB505 3 arcsec diameter aperture flux density error (SC\_IB505ap3)uJystat.error;phot.flux.density;em.opt.VfloatnullableFSCIB505?=- SC_IB505 AUTO flux density (SC\_IB505\_FLUX_AUTO)uJyphot.flux.density;em.opt.Vfloatnullablee_FSCIB505?=- SC_IB505 AUTO flux density error (SC\_IB505\_FLUXERR_AUTO)uJystat.error;phot.flux.density;em.opt.VfloatnullableSCIB505magap2?=- SC_IB505 2 arcsec diameter aperture AB magnitude (SC\_IB505\_MAG_APER2)magphot.mag;em.opt.Vfloatnullablee_SCIB505magap2?=- SC_IB505 2 arcsec diameter aperture AB magnitude error (SC\_IB505\_MAGERR_APER2)magstat.error;phot.mag;em.opt.VdoublenullableSCIB505magap3?=- SC_IB505 3 arcsec diameter aperture AB magnitude (SC\_IB505\_MAG_APER3)magphot.mag;em.opt.Vfloatnullablee_SCIB505magap3?=- SC_IB505 3 arcsec diameter aperture AB magnitude error (SC\_IB505\_MAGERR_APER3)magstat.error;phot.mag;em.opt.VdoublenullableSCIB505magAuto?=- SC_IB505 AUTO AB magnitude (SC\_IB505\_MAG_AUTO)magphot.mag;em.opt.Vfloatnullablee_SCIB505magAuto?=- SC_IB505 AUTO AB magnitude error (SC\_IB505\_MAGERR_AUTO)magstat.error;phot.mag;em.opt.VdoublenullableSCIB505magIso?=- SC_IB505 ISO AB magnitude (SC\_IB505\_MAG_ISO)magphot.mag;em.opt.Vfloatnullablee_SCIB505magIso?=- SC_IB505 ISO AB magnitude error (SC\_IB505\_MAGERR_ISO)magstat.error;phot.mag;em.opt.VdoublenullableSCIB505Flag?=- SC_IB505 Source Extractor internal flags (SC\_IB505\_FLAGS)meta.code;phot;em.opt.VintnullableSCIB505FlagIso?=- SC_IB505 flags: 4 means saturated pixel (s) in the isophotal area (SC\_IB505\_IMAFLAGS_ISO)meta.code;phot;em.opt.VintnullableFSCIA527ap2?=- SC_IA527 2 arcsec diameter aperture flux density (SC\_IA527\_FLUX_APER2)uJyphot.flux.density;em.opt.Vdoublenullablee_FSCIA527ap2?=- SC_IA527 2 arcsec diameter aperture flux density error (SC\_IA527\_FLUXERR_APER2)uJystat.error;phot.flux.density;em.opt.VfloatnullableFSCIA527ap3?=- SC_IA527 3 arcsec diameter aperture flux density (SC\_IA527\_FLUX_APER3)uJyphot.flux.density;em.opt.Vdoublenullablee_FSCIA527ap3?=- SC_IA527 3 arcsec diameter aperture flux density error (SC\_IA527ap3)uJystat.error;phot.flux.density;em.opt.VfloatnullableFSCIA527?=- SC_IA527 AUTO flux density (SC\_IA527\_FLUX_AUTO)uJyphot.flux.density;em.opt.Vdoublenullablee_FSCIA527?=- SC_IA527 AUTO flux density error (SC\_IA527\_FLUXERR_AUTO)uJystat.error;phot.flux.density;em.opt.VfloatnullableSCIA527magap2?=- SC_IA527 2 arcsec diameter aperture AB magnitude (SC\_IA527\_MAG_APER2)magphot.mag;em.opt.Vfloatnullablee_SCIA527magap2?=- SC_IA527 2 arcsec diameter aperture AB magnitude error (SC\_IA527\_MAGERR_APER2)magstat.error;phot.mag;em.opt.VdoublenullableSCIA527magap3?=- SC_IA527 3 arcsec diameter aperture AB magnitude (SC\_IA527\_MAG_APER3)magphot.mag;em.opt.Vfloatnullablee_SCIA527magap3?=- SC_IA527 3 arcsec diameter aperture AB magnitude error (SC\_IA527\_MAGERR_APER3)magstat.error;phot.mag;em.opt.VdoublenullableSCIA527magAuto?=- SC_IA527 AUTO AB magnitude (SC\_IA527\_MAG_AUTO)magphot.mag;em.opt.Vfloatnullablee_SCIA527magAuto?=- SC_IA527 AUTO AB magnitude error (SC\_IA527\_MAGERR_AUTO)magstat.error;phot.mag;em.opt.VdoublenullableSCIA527magIso?=- SC_IA527 ISO AB magnitude (SC\_IA527\_MAG_ISO)magphot.mag;em.opt.Vfloatnullablee_SCIA527magIso?=- SC_IA527 ISO AB magnitude error (SC\_IA527\_MAGERR_ISO)magstat.error;phot.mag;em.opt.VdoublenullableSCIA527Flag?=- SC_IA527 Source Extractor internal flags (SC\_IA527\_FLAGS)meta.code;phot;em.opt.VintnullableSCIA527FlagIso?=- SC_IA527 flags: 4 means saturated pixel (s) in the isophotal area (SC\_IA527\_IMAFLAGS_ISO)meta.code;phot;em.opt.VintnullableFSCIB574ap2?=- SC_IB574 2 arcsec diameter aperture flux density (SC\_IB574\_FLUX_APER2)uJyphot.flux.density;em.opt.Vfloatnullablee_FSCIB574ap2?=- SC_IB574 2 arcsec diameter aperture flux density error (SC\_IB574\_FLUXERR_APER2)uJystat.error;phot.flux.density;em.opt.VfloatnullableFSCIB574ap3?=- SC_IB574 3 arcsec diameter aperture flux density (SC\_IB574\_FLUX_APER3)uJyphot.flux.density;em.opt.Vfloatnullablee_FSCIB574ap3?=- SC_IB574 3 arcsec diameter aperture flux density error (SC\_IB574ap3)uJystat.error;phot.flux.density;em.opt.VfloatnullableFSCIB574?=- SC_IB574 AUTO flux density (SC\_IB574\_FLUX_AUTO)uJyphot.flux.density;em.opt.Vdoublenullablee_FSCIB574?=- SC_IB574 AUTO flux density error (SC\_IB574\_FLUXERR_AUTO)uJystat.error;phot.flux.density;em.opt.VfloatnullableSCIB574magap2?=- SC_IB574 2 arcsec diameter aperture AB magnitude (SC\_IB574\_MAG_APER2)magphot.mag;em.opt.Vfloatnullablee_SCIB574magap2?=- SC_IB574 2 arcsec diameter aperture AB magnitude error (SC\_IB574\_MAGERR_APER2)magstat.error;phot.mag;em.opt.VdoublenullableSCIB574magap3?=- SC_IB574 3 arcsec diameter aperture AB magnitude (SC\_IB574\_MAG_APER3)magphot.mag;em.opt.Vfloatnullablee_SCIB574magap3?=- SC_IB574 3 arcsec diameter aperture AB magnitude error (SC\_IB574\_MAGERR_APER3)magstat.error;phot.mag;em.opt.VdoublenullableSCIB574magAuto?=- SC_IB574 AUTO AB magnitude (SC\_IB574\_MAG_AUTO)magphot.mag;em.opt.Vfloatnullablee_SCIB574magAuto?=- SC_IB574 AUTO AB magnitude error (SC\_IB574\_MAGERR_AUTO)magstat.error;phot.mag;em.opt.VdoublenullableSCIB574magIso?=- SC_IB574 ISO AB magnitude (SC\_IB574\_MAG_ISO)magphot.mag;em.opt.Vfloatnullablee_SCIB574magIso?=- SC_IB574 ISO AB magnitude error (SC\_IB574\_MAGERR_ISO)magstat.error;phot.mag;em.opt.VdoublenullableSCIB574Flag?=- SC_IB574 Source Extractor internal flags (SC\_IB574\_FLAGS)meta.code;phot;em.opt.VintnullableSCIB574FlagIso?=- SC_IB574 flags: 4 means saturated pixel (s) in the isophotal area (SC\_IB574\_IMAFLAGS_ISO)meta.code;phot;em.opt.VintnullableFSCIA624ap2?=- SC_IA624 2 arcsec diameter aperture flux density (SC\_IA624\_FLUX_APER2)uJyphot.flux.density;em.opt.Rdoublenullablee_FSCIA624ap2?=- SC_IA624 2 arcsec diameter aperture flux density error (SC\_IA624\_FLUXERR_APER2)uJystat.error;phot.flux.density;em.opt.RfloatnullableFSCIA624ap3?=- SC_IA624 3 arcsec diameter aperture flux density (SC\_IA624\_FLUX_APER3)uJyphot.flux.density;em.opt.Rdoublenullablee_FSCIA624ap3?=- SC_IA624 3 arcsec diameter aperture flux density error (SC\_IA624ap3)uJystat.error;phot.flux.density;em.opt.RfloatnullableFSCIA624?=- SC_IA624 AUTO flux density (SC\_IA624\_FLUX_AUTO)uJyphot.flux.density;em.opt.Rdoublenullablee_FSCIA624?=- SC_IA624 AUTO flux density error (SC\_IA624\_FLUXERR_AUTO)uJystat.error;phot.flux.density;em.opt.RfloatnullableSCIA624magap2?=- SC_IA624 2 arcsec diameter aperture AB magnitude (SC\_IA624\_MAG_APER2)magphot.mag;em.opt.Rfloatnullablee_SCIA624magap2?=- SC_IA624 2 arcsec diameter aperture AB magnitude error (SC\_IA624\_MAGERR_APER2)magstat.error;phot.mag;em.opt.RdoublenullableSCIA624magap3?=- SC_IA624 3 arcsec diameter aperture AB magnitude (SC\_IA624\_MAG_APER3)magphot.mag;em.opt.Rfloatnullablee_SCIA624magap3?=- SC_IA624 3 arcsec diameter aperture AB magnitude error (SC\_IA624\_MAGERR_APER3)magstat.error;phot.mag;em.opt.RdoublenullableSCIA624magAuto?=- SC_IA624 AUTO AB magnitude (SC\_IA624\_MAG_AUTO)magphot.mag;em.opt.Rfloatnullablee_SCIA624magAuto?=- SC_IA624 AUTO AB magnitude error (SC\_IA624\_MAGERR_AUTO)magstat.error;phot.mag;em.opt.RdoublenullableSCIA624magIso?=- SC_IA624 ISO AB magnitude (SC\_IA624\_MAG_ISO)magphot.mag;em.opt.Rfloatnullablee_SCIA624magIso?=- SC_IA624 ISO AB magnitude error (SC\_IA624\_MAGERR_ISO)magstat.error;phot.mag;em.opt.RdoublenullableSCIA624Flag?=- SC_IA624 Source Extractor internal flags (SC\_IA624\_FLAGS)meta.code;phot;em.opt.RintnullableSCIA624FlagIso?=- SC_IA624 flags: 4 means saturated pixel (s) in the isophotal area (SC\_IA624\_IMAFLAGS_ISO)meta.code;phot;em.opt.RintnullableFSCIA679ap2?=- SC_IA679 2 arcsec diameter aperture flux density (SC\_IA679\_FLUX_APER2)uJyphot.flux.density;em.opt.Rdoublenullablee_FSCIA679ap2?=- SC_IA679 2 arcsec diameter aperture flux density error (SC\_IA679\_FLUXERR_APER2)uJystat.error;phot.flux.density;em.opt.RfloatnullableFSCIA679ap3?=- SC_IA679 3 arcsec diameter aperture flux density (SC\_IA679\_FLUX_APER3)uJyphot.flux.density;em.opt.Rdoublenullablee_FSCIA679ap3?=- SC_IA679 3 arcsec diameter aperture flux density error (SC\_IA679ap3)uJystat.error;phot.flux.density;em.opt.RfloatnullableFSCIA679?=- SC_IA679 AUTO flux density (SC\_IA679\_FLUX_AUTO)uJyphot.flux.density;em.opt.Rdoublenullablee_FSCIA679?=- SC_IA679 AUTO flux density error (SC\_IA679\_FLUXERR_AUTO)uJystat.error;phot.flux.density;em.opt.RfloatnullableSCIA679magap2?=- SC_IA679 2 arcsec diameter aperture AB magnitude (SC\_IA679\_MAG_APER2)magphot.mag;em.opt.Rfloatnullablee_SCIA679magap2?=- SC_IA679 2 arcsec diameter aperture AB magnitude error (SC\_IA679\_MAGERR_APER2)magstat.error;phot.mag;em.opt.RdoublenullableSCIA679magap3?=- SC_IA679 3 arcsec diameter aperture AB magnitude (SC\_IA679\_MAG_APER3)magphot.mag;em.opt.Rfloatnullablee_SCIA679magap3?=- SC_IA679 3 arcsec diameter aperture AB magnitude error (SC\_IA679\_MAGERR_APER3)magstat.error;phot.mag;em.opt.RdoublenullableSCIA679magAuto?=- SC_IA679 AUTO AB magnitude (SC\_IA679\_MAG_AUTO)magphot.mag;em.opt.Rfloatnullablee_SCIA679magAuto?=- SC_IA679 AUTO AB magnitude error (SC\_IA679\_MAGERR_AUTO)magstat.error;phot.mag;em.opt.RdoublenullableSCIA679magIso?=- SC_IA679 ISO AB magnitude (SC\_IA679\_MAG_ISO)magphot.mag;em.opt.Rfloatnullablee_SCIA679magIso?=- SC_IA679 ISO AB magnitude error (SC\_IA679\_MAGERR_ISO)magstat.error;phot.mag;em.opt.RdoublenullableSCIA679Flag?=- SC_IA679 Source Extractor internal flags (SC\_IA679\_FLAGS)meta.code;phot;em.opt.RintnullableSCIA679FlagIso?=- SC_IA679 flags: 4 means saturated pixel (s) in the isophotal area (SC\_IA679\_IMAFLAGS_ISO)meta.code;phot;em.opt.RintnullableFSCIB709ap2?=- SC_IB709 2 arcsec diameter aperture flux density (SC\_IB709\_FLUX_APER2)uJyphot.flux.density;em.opt.Rfloatnullablee_FSCIB709ap2?=- SC_IB709 2 arcsec diameter aperture flux density error (SC\_IB709\_FLUXERR_APER2)uJystat.error;phot.flux.density;em.opt.RfloatnullableFSCIB709ap3?=- SC_IB709 3 arcsec diameter aperture flux density (SC\_IB709\_FLUX_APER3)uJyphot.flux.density;em.opt.Rfloatnullablee_FSCIB709ap3?=- SC_IB709 3 arcsec diameter aperture flux density error (SC\_IB709ap3)uJystat.error;phot.flux.density;em.opt.RfloatnullableFSCIB709?=- SC_IB709 AUTO flux density (SC\_IB709\_FLUX_AUTO)uJyphot.flux.density;em.opt.Rfloatnullablee_FSCIB709?=- SC_IB709 AUTO flux density error (SC\_IB709\_FLUXERR_AUTO)uJystat.error;phot.flux.density;em.opt.RfloatnullableSCIB709magap2?=- SC_IB709 2 arcsec diameter aperture AB magnitude (SC\_IB709\_MAG_APER2)magphot.mag;em.opt.Rfloatnullablee_SCIB709magap2?=- SC_IB709 2 arcsec diameter aperture AB magnitude error (SC\_IB709\_MAGERR_APER2)magstat.error;phot.mag;em.opt.RdoublenullableSCIB709magap3?=- SC_IB709 3 arcsec diameter aperture AB magnitude (SC\_IB709\_MAG_APER3)magphot.mag;em.opt.Rfloatnullablee_SCIB709magap3?=- SC_IB709 3 arcsec diameter aperture AB magnitude error (SC\_IB709\_MAGERR_APER3)magstat.error;phot.mag;em.opt.RdoublenullableSCIB709magAuto?=- SC_IB709 AUTO AB magnitude (SC\_IB709\_MAG_AUTO)magphot.mag;em.opt.Rfloatnullablee_SCIB709magAuto?=- SC_IB709 AUTO AB magnitude error (SC\_IB709\_MAGERR_AUTO)magstat.error;phot.mag;em.opt.RdoublenullableSCIB709magIso?=- SC_IB709 ISO AB magnitude (SC\_IB709\_MAG_ISO)magphot.mag;em.opt.Rfloatnullablee_SCIB709magIso?=- SC_IB709 ISO AB magnitude error (SC\_IB709\_MAGERR_ISO)magstat.error;phot.mag;em.opt.RdoublenullableSCIB709Flag?=- SC_IB709 Source Extractor internal flags (SC\_IB709\_FLAGS)meta.code;phot;em.opt.RintnullableUVISTANB118Flag?=- UVISTA_NB118 Source Extractor internal flags (UVISTA\_NB118\_FLAGS)phot.mag;em.IR.JintnullableSCIB709FlagIso?=- SC_IB709 flags: 4 means saturated pixel (s) in the isophotal area (SC\_IB709\_IMAFLAGS_ISO)meta.code;phot;em.opt.RintnullableFSCIA738ap2?=- SC_IA738 2 arcsec diameter aperture flux density (SC\_IA738\_FLUX_APER2)uJyphot.flux.density;em.opt.Rfloatnullablee_FSCIA738ap2?=- SC_IA738 2 arcsec diameter aperture flux density error (SC\_IA738\_FLUXERR_APER2)uJystat.error;phot.flux.density;em.opt.RfloatnullableFSCIA738ap3?=- SC_IA738 3 arcsec diameter aperture flux density (SC\_IA738\_FLUX_APER3)uJyphot.flux.density;em.opt.Rfloatnullablee_FSCIA738ap3?=- SC_IA738 3 arcsec diameter aperture flux density error (SC\_IA738ap3)uJystat.error;phot.flux.density;em.opt.RfloatnullableFSCIA738?=- SC_IA738 AUTO flux density (SC\_IA738\_FLUX_AUTO)uJyphot.flux.density;em.opt.Rfloatnullablee_FSCIA738?=- SC_IA738 AUTO flux density error (SC\_IA738\_FLUXERR_AUTO)uJystat.error;phot.flux.density;em.opt.RfloatnullableSCIA738magap2?=- SC_IA738 2 arcsec diameter aperture AB magnitude (SC\_IA738\_MAG_APER2)magphot.mag;em.opt.Rfloatnullablee_SCIA738magap2?=- SC_IA738 2 arcsec diameter aperture AB magnitude error (SC\_IA738\_MAGERR_APER2)magstat.error;phot.mag;em.opt.RdoublenullableSCIA738magap3?=- SC_IA738 3 arcsec diameter aperture AB magnitude (SC\_IA738\_MAG_APER3)magphot.mag;em.opt.Rfloatnullablee_SCIA738magap3?=- SC_IA738 3 arcsec diameter aperture AB magnitude error (SC\_IA738\_MAGERR_APER3)magstat.error;phot.mag;em.opt.RdoublenullableSCIA738magAuto?=- SC_IA738 AUTO AB magnitude (SC\_IA738\_MAG_AUTO)magphot.mag;em.opt.Rfloatnullablee_SCIA738magAuto?=- SC_IA738 AUTO AB magnitude error (SC\_IA738\_MAGERR_AUTO)magstat.error;phot.mag;em.opt.RdoublenullableSCIA738magIso?=- SC_IA738 ISO AB magnitude (SC\_IA738\_MAG_ISO)magphot.mag;em.opt.Rfloatnullablee_SCIA738magIso?=- SC_IA738 ISO AB magnitude error (SC\_IA738\_MAGERR_ISO)magstat.error;phot.mag;em.opt.RdoublenullableSCIA738Flag?=- SC_IA738 Source Extractor internal flags (SC\_IA738\_FLAGS)meta.code;phot;em.opt.RintnullableSCIA738FlagIso?=- SC_IA738 flags: 4 means saturated pixel (s) in the isophotal area (SC\_IA738\_IMAFLAGS_ISO)meta.code;phot;em.opt.RintnullableFSCIA767ap2?=- SC_IA767 2 arcsec diameter aperture flux density (SC\_IA767\_FLUX_APER2)uJyphot.flux.density;em.opt.Idoublenullablee_FSCIA767ap2?=- SC_IA767 2 arcsec diameter aperture flux density error (SC\_IA767\_FLUXERR_APER2)uJystat.error;phot.flux.density;em.opt.IfloatnullableFSCIA767ap3?=- SC_IA767 3 arcsec diameter aperture flux density (SC\_IA767\_FLUX_APER3)uJyphot.flux.density;em.opt.Idoublenullablee_FSCIA767ap3?=- SC_IA767 3 arcsec diameter aperture flux density error (SC\_IA767ap3)uJystat.error;phot.flux.density;em.opt.IfloatnullableFSCIA767?=- SC_IA767 AUTO flux density (SC\_IA767\_FLUX_AUTO)uJyphot.flux.density;em.opt.Idoublenullablee_FSCIA767?=- SC_IA767 AUTO flux density error (SC\_IA767\_FLUXERR_AUTO)uJystat.error;phot.flux.density;em.opt.IfloatnullableSCIA767magap2?=- SC_IA767 2 arcsec diameter aperture AB magnitude (SC\_IA767\_MAG_APER2)magphot.mag;em.opt.Ifloatnullablee_SCIA767magap2?=- SC_IA767 2 arcsec diameter aperture AB magnitude error (SC\_IA767\_MAGERR_APER2)magstat.error;phot.mag;em.opt.IdoublenullableSCIA767magap3?=- SC_IA767 3 arcsec diameter aperture AB magnitude (SC\_IA767\_MAG_APER3)magphot.mag;em.opt.Ifloatnullablee_SCIA767magap3?=- SC_IA767 3 arcsec diameter aperture AB magnitude error (SC\_IA767\_MAGERR_APER3)magstat.error;phot.mag;em.opt.IdoublenullableSCIA767magAuto?=- SC_IA767 AUTO AB magnitude (SC\_IA767\_MAG_AUTO)magphot.mag;em.opt.Ifloatnullablee_SCIA767magAuto?=- SC_IA767 AUTO AB magnitude error (SC\_IA767\_MAGERR_AUTO)magstat.error;phot.mag;em.opt.IdoublenullableSCIA767magIso?=- SC_IA767 ISO AB magnitude (SC\_IA767\_MAG_ISO)magphot.mag;em.opt.Ifloatnullablee_SCIA767magIso?=- SC_IA767 ISO AB magnitude error (SC\_IA767\_MAGERR_ISO)magstat.error;phot.mag;em.opt.IdoublenullableSCIA767Flag?=- SC_IA767 Source Extractor internal flags (SC\_IA767\_FLAGS)meta.code;phot;em.opt.Iintnullablee_FSCVap2?=- SC_V 2 arcsec diameter aperture flux density error (SC\_V\_FLUXERR_APER2)uJystat.error;phot.flux.density;em.opt.VfloatnullableSCIA767FlagIso?=- SC_IA767 flags: 4 means saturated pixel (s) in the isophotal area (SC\_IA767\_IMAFLAGS_ISO)meta.code;phot;em.opt.IintnullableFSCIB827ap2?=- SC_IB827 2 arcsec diameter aperture flux density (SC\_IB827\_FLUX_APER2)uJyphot.flux.density;em.opt.Ifloatnullablee_FSCIB827ap2?=- SC_IB827 2 arcsec diameter aperture flux density error (SC\_IB827\_FLUXERR_APER2)uJystat.error;phot.flux.density;em.opt.IfloatnullableFSCIB827ap3?=- SC_IB827 3 arcsec diameter aperture flux density (SC\_IB827\_FLUX_APER3)uJyphot.flux.density;em.opt.Ifloatnullablee_FSCIB827ap3?=- SC_IB827 3 arcsec diameter aperture flux density error (SC\_IB827ap3)uJystat.error;phot.flux.density;em.opt.IfloatnullableFSCIB827?=- SC_IB827 AUTO flux density (SC\_IB827\_FLUX_AUTO)uJyphot.flux.density;em.opt.Idoublenullablee_FSCIB827?=- SC_IB827 AUTO flux density error (SC\_IB827\_FLUXERR_AUTO)uJystat.error;phot.flux.density;em.opt.IfloatnullableSCIB827magap2?=- SC_IB827 2 arcsec diameter aperture AB magnitude (SC\_IB827\_MAG_APER2)magphot.mag;em.opt.Ifloatnullablee_SCIB827magap2?=- SC_IB827 2 arcsec diameter aperture AB magnitude error (SC\_IB827\_MAGERR_APER2)magstat.error;phot.mag;em.opt.IdoublenullableSCIB827magap3?=- SC_IB827 3 arcsec diameter aperture AB magnitude (SC\_IB827\_MAG_APER3)magphot.mag;em.opt.Ifloatnullablee_SCIB827magap3?=- SC_IB827 3 arcsec diameter aperture AB magnitude error (SC\_IB827\_MAGERR_APER3)magstat.error;phot.mag;em.opt.IdoublenullableSCIB827magAuto?=- SC_IB827 AUTO AB magnitude (SC\_IB827\_MAG_AUTO)magphot.mag;em.opt.Ifloatnullablee_SCIB827magAuto?=- SC_IB827 AUTO AB magnitude error (SC\_IB827\_MAGERR_AUTO)magstat.error;phot.mag;em.opt.IdoublenullableSCIB827magIso?=- SC_IB827 ISO AB magnitude (SC\_IB827\_MAG_ISO)magphot.mag;em.opt.Ifloatnullablee_SCIB827magIso?=- SC_IB827 ISO AB magnitude error (SC\_IB827\_MAGERR_ISO)magstat.error;phot.mag;em.opt.IdoublenullableSCIB827Flag?=- SC_IB827 Source Extractor internal flags (SC\_IB827\_FLAGS)meta.code;phot;em.opt.IintnullableSCIB827FlagIso?=- SC_IB827 flags: 4 means saturated pixel (s) in the isophotal area (SC\_IB827\_IMAFLAGS_ISO)meta.code;phot;em.opt.IintnullableFSCNB711ap2?=- SC_NB711 2 arcsec diameter aperture flux density (SC\_NB711\_FLUX_APER2)uJyphot.flux.density;em.opt.Rfloatnullablee_FSCNB711ap2?=- SC_NB711 2 arcsec diameter aperture flux density error (SC\_NB711\_FLUXERR_APER2)uJystat.error;phot.flux.density;em.opt.RfloatnullableFSCNB711ap3?=- SC_NB711 3 arcsec diameter aperture flux density (SC\_NB711\_FLUX_APER3)uJyphot.flux.density;em.opt.Rfloatnullablee_FSCNB711ap3?=- SC_NB711 3 arcsec diameter aperture flux density error (SC\_NB711ap3)uJystat.error;phot.flux.density;em.opt.RfloatnullableFSCNB711?=- SC_NB711 AUTO flux density (SC\_NB711\_FLUX_AUTO)uJyphot.flux.density;em.opt.Rdoublenullablee_FSCNB711?=- SC_NB711 AUTO flux density error (SC\_NB711\_FLUXERR_AUTO)uJystat.error;phot.flux.density;em.opt.RfloatnullableSCNB711magap2?=- SC_NB711 2 arcsec diameter aperture AB magnitude (SC\_NB711\_MAG_APER2)magphot.mag;em.opt.Rfloatnullablee_SCNB711magap2?=- SC_NB711 2 arcsec diameter aperture AB magnitude error (SC\_NB711\_MAGERR_APER2)magstat.error;phot.mag;em.opt.RdoublenullableSCNB711magap3?=- SC_NB711 3 arcsec diameter aperture AB magnitude (SC\_NB711\_MAG_APER3)magphot.mag;em.opt.Rfloatnullablee_SCNB711magap3?=- SC_NB711 3 arcsec diameter aperture AB magnitude error (SC\_NB711\_MAGERR_APER3)magstat.error;phot.mag;em.opt.RdoublenullableSCNB711magAuto?=- SC_NB711 AUTO AB magnitude (SC\_NB711\_MAG_AUTO)magphot.mag;em.opt.Rfloatnullablee_SCNB711magAuto?=- SC_NB711 AUTO AB magnitude error (SC\_NB711\_MAGERR_AUTO)magstat.error;phot.mag;em.opt.RdoublenullableSCNB711magIso?=- SC_NB711 ISO AB magnitude (SC\_NB711\_MAG_ISO)magphot.mag;em.opt.Rfloatnullablee_SCNB711magIso?=- SC_NB711 ISO AB magnitude error (SC\_NB711\_MAGERR_ISO)magstat.error;phot.mag;em.opt.RdoublenullableSCNB711Flag?=- SC_NB711 Source Extractor internal flags (SC\_NB711\_FLAGS)meta.code;phot;em.opt.RintnullableFSCVap3?=- SC_V 3 arcsec diameter aperture flux density (SC\_V\_FLUX_APER3)uJyphot.flux.density;em.opt.VfloatnullableSCNB711FlagIso?=- SC_NB711 flags: 4 means saturated pixel (s) in the isophotal area (SC\_NB711\_IMAFLAGS_ISO)meta.code;phot;em.opt.RintnullableFSCNB816ap2?=- SC_NB816 2 arcsec diameter aperture flux density (SC\_NB816\_FLUX_APER2)uJyphot.flux.density;em.opt.Ifloatnullablee_FSCNB816ap2?=- SC_NB816 2 arcsec diameter aperture flux density error (SC\_NB816\_FLUXERR_APER2)uJystat.error;phot.flux.density;em.opt.IfloatnullableFSCNB816ap3?=- SC_NB816 3 arcsec diameter aperture flux density (SC\_NB816\_FLUX_APER3)uJyphot.flux.density;em.opt.Idoublenullablee_FSCNB816ap3?=- SC_NB816 3 arcsec diameter aperture flux density error (SC\_NB816ap3)uJystat.error;phot.flux.density;em.opt.IfloatnullableFSCNB816?=- SC_NB816 AUTO flux density (SC\_NB816\_FLUX_AUTO)uJyphot.flux.density;em.opt.Idoublenullablee_FSCNB816?=- SC_NB816 AUTO flux density error (SC\_NB816\_FLUXERR_AUTO)uJystat.error;phot.flux.density;em.opt.IfloatnullableSCNB816magap2?=- SC_NB816 2 arcsec diameter aperture AB magnitude (SC\_NB816\_MAG_APER2)magphot.mag;em.opt.Ifloatnullablee_SCNB816magap2?=- SC_NB816 2 arcsec diameter aperture AB magnitude error (SC\_NB816\_MAGERR_APER2)magstat.error;phot.mag;em.opt.IdoublenullableSCNB816magap3?=- SC_NB816 3 arcsec diameter aperture AB magnitude (SC\_NB816\_MAG_APER3)magphot.mag;em.opt.Ifloatnullablee_SCNB816magap3?=- SC_NB816 3 arcsec diameter aperture AB magnitude error (SC\_NB816\_MAGERR_APER3)magstat.error;phot.mag;em.opt.IdoublenullableSCNB816magAuto?=- SC_NB816 AUTO AB magnitude (SC\_NB816\_MAG_AUTO)magphot.mag;em.opt.Ifloatnullablee_SCNB816magAuto?=- SC_NB816 AUTO AB magnitude error (SC\_NB816\_MAGERR_AUTO)magstat.error;phot.mag;em.opt.IdoublenullableSCNB816magIso?=- SC_NB816 ISO AB magnitude (SC\_NB816\_MAG_ISO)magphot.mag;em.opt.Ifloatnullablee_SCNB816magIso?=- SC_NB816 ISO AB magnitude error (SC\_NB816\_MAGERR_ISO)magstat.error;phot.mag;em.opt.IdoublenullableSCNB816Flag?=- SC_NB816 Source Extractor internal flags (SC\_NB816\_FLAGS)meta.code;phot;em.opt.IintnullableSCNB816FlagIso?=- SC_NB816 flags: 4 means saturated pixel (s) in the isophotal area (SC\_NB816\_IMAFLAGS_ISO)meta.code;phot;em.opt.IintnullableFUVISTANB118ap2?=- UVISTA_NB118 2 arcsec diameter aperture flux density (UVISTA\_NB118\_FLUX_APER2)uJyphot.flux.density;em.IR.Jdoublenullablee_FUVISTANB118ap2?=- UVISTA_NB118 2 arcsec diameter aperture flux density error (UVISTA\_NB118\_FLUXERR_APER2)uJystat.error;phot.flux.density;em.IR.JfloatnullableFUVISTANB118ap3?=- UVISTA_NB118 3 arcsec diameter aperture flux density (UVISTA\_NB118\_FLUX_APER3)uJyphot.flux.density;em.IR.Jdoublenullablee_FUVISTANB118ap3?=- UVISTA_NB118 3 arcsec diameter aperture flux density error (UVISTA\_NB118\_FLUXERR_APER3)uJystat.error;phot.flux.density;em.IR.JfloatnullableFUVISTANB118?=- UVISTA_NB118 AUTO flux density (UVISTA\_NB118\_FLUX_AUTO)uJyphot.flux.density;em.IR.Jdoublenullablee_FUVISTANB118?=- UVISTA_NB118 AUTO flux density error (UVISTA\_NB118\_FLUXERR_AUTO)uJystat.error;phot.flux.density;em.IR.JfloatnullableUVISTANB118magap2?=- UVISTA_NB118 2 arcsec diameter aperture AB magnitude (UVISTA\_NB118\_MAG_APER2)magphot.mag;em.IR.Jfloatnullablee_UVISTANB118magap2?=- UVISTA_NB118 2 arcsec diameter aperture AB magnitude error (UVISTA\_NB118\_MAGERR_APER2)magstat.error;phot.mag;em.IR.JdoublenullableUVISTANB118magap3?=- UVISTA_NB118 3 arcsec diameter aperture AB magnitude (UVISTA\_NB118\_MAG_APER3)magphot.mag;em.IR.Jfloatnullablee_UVISTANB118magap3?=- UVISTA_NB118 3 arcsec diameter aperture AB magnitude error (UVISTA\_NB118\_MAGERR_APER3)magstat.error;phot.mag;em.IR.JdoublenullableUVISTANB118magAuto?=- UVISTA_NB118 AUTO AB magnitude (UVISTA\_NB118\_MAG_AUTO)magphot.mag;em.IR.Jfloatnullablee_UVISTANB118magAuto?=- UVISTA_NB118 AUTO AB magnitude error (UVISTA\_NB118\_MAGERR_AUTO)magstat.error;phot.mag;em.IR.JdoublenullableUVISTANB118magIso?=- UVISTA_NB118 ISO AB magnitude (UVISTA\_NB118\_MAG_ISO)magphot.mag;em.IR.Jfloatnullablee_UVISTANB118magIso?=- UVISTA_NB118 ISO AB magnitude error (UVISTA\_NB118\_MAGERR_ISO)magstat.error;phot.mag;em.IR.JdoublenullableUVISTANB118FlagIso?=- UVISTA_NB118 flags: 4 means saturated pixel (s) in the isophotal area (UVISTA\_NB118\_IMAFLAGS_ISO)phot.mag;em.IR.JintnullableFSCBap2?=- SC_B 2 arcsec diameter aperture flux density (SC\_B\_FLUX_APER2)uJyphot.flux.density;em.opt.Bfloatnullablee_FSCBap2?=- SC_B 2 arcsec diameter aperture flux density error (SC\_B\_FLUXERR_APER2)uJystat.error;phot.flux.density;em.opt.BfloatnullableFSCBap3?=- SC_B 3 arcsec diameter aperture flux density (SC\_B\_FLUX_APER3)uJyphot.flux.density;em.opt.Bfloatnullablee_FSCBap3?=- SC_B 3 arcsec diameter aperture flux density error (SC\_Bap3)uJystat.error;phot.flux.density;em.opt.BfloatnullableFSCB?=- SC_B AUTO flux density (SC\_B\_FLUX_AUTO)uJyphot.flux.density;em.opt.Bfloatnullablee_FSCB?=- SC_B AUTO flux density error (SC\_B\_FLUXERR_AUTO)uJystat.error;phot.flux.density;em.opt.BfloatnullableSCBmagap2?=- SC_B 2 arcsec diameter aperture AB magnitude (SC\_B\_MAG_APER2)magphot.mag;em.opt.Bfloatnullablee_SCBmagap2?=- SC_B 2 arcsec diameter aperture AB magnitude error (SC\_B\_MAGERR_APER2)magstat.error;phot.mag;em.opt.BdoublenullableSCBmagap3?=- SC_B 3 arcsec diameter aperture AB magnitude (SC\_B\_MAG_APER3)magphot.mag;em.opt.Bfloatnullablee_SCBmagap3?=- SC_B 3 arcsec diameter aperture AB magnitude error (SC\_B\_MAGERR_APER3)magstat.error;phot.mag;em.opt.BdoublenullableSCBmagAuto?=- SC_B AUTO AB magnitude (SC\_B\_MAG_AUTO)magphot.mag;em.opt.Bfloatnullablee_SCBmagAuto?=- SC_B AUTO AB magnitude error (SC\_B\_MAGERR_AUTO)magstat.error;phot.mag;em.opt.Bdoublenullablee_SCBmagIso?=- SC_B ISO AB magnitude error (SC\_B\_MAGERR_ISO)magstat.error;phot.mag;em.opt.BdoublenullableSCBFlag?=- SC_B Source Extractor internal flags (SC\_B\_FLAGS)meta.code;phot;em.opt.Bintnullablee_FSCzp?=- SC_zp AUTO flux density error (SC\_zp\_FLUXERR_AUTO)uJystat.error;phot.flux.density;em.opt.IfloatnullableSCBFlagIso?=- SC_B flags: 4 means saturated pixel (s) in the isophotal area (SC\_B\_IMAFLAGS_ISO)meta.code;phot;em.opt.BintnullableFSCgpap2?=- SC_gp 2 arcsec diameter aperture flux density (SC\_gp\_FLUX_APER2)uJyphot.flux.density;em.opt.Bfloatnullablee_FSCgpap2?=- SC_gp 2 arcsec diameter aperture flux density error (SC\_gp\_FLUXERR_APER2)uJystat.error;phot.flux.density;em.opt.BfloatnullableFSCgpap3?=- SC_gp 3 arcsec diameter aperture flux density (SC\_gp\_FLUX_APER3)uJyphot.flux.density;em.opt.Bfloatnullablee_FSCgpap3?=- SC_gp 3 arcsec diameter aperture flux density error (SC\_gpap3)uJystat.error;phot.flux.density;em.opt.BfloatnullableFSCgp?=- SC_gp AUTO flux density (SC\_gp\_FLUX_AUTO)uJyphot.flux.density;em.opt.Bfloatnullablee_FSCgp?=- SC_gp AUTO flux density error (SC\_gp\_FLUXERR_AUTO)uJystat.error;phot.flux.density;em.opt.BfloatnullableSCgpmagap2?=- SC_gp 2 arcsec diameter aperture AB magnitude (SC\_gp\_MAG_APER2)magphot.mag;em.opt.Bfloatnullablee_SCgpmagap2?=- SC_gp 2 arcsec diameter aperture AB magnitude error (SC\_gp\_MAGERR_APER2)magstat.error;phot.mag;em.opt.BdoublenullableSCgpmagap3?=- SC_gp 3 arcsec diameter aperture AB magnitude (SC\_gp\_MAG_APER3)magphot.mag;em.opt.Bfloatnullablee_SCgpmagap3?=- SC_gp 3 arcsec diameter aperture AB magnitude error (SC\_gp\_MAGERR_APER3)magstat.error;phot.mag;em.opt.BdoublenullableSCgpmagAuto?=- SC_gp AUTO AB magnitude (SC\_gp\_MAG_AUTO)magphot.mag;em.opt.Bfloatnullablee_SCgpmagAuto?=- SC_gp AUTO AB magnitude error (SC\_gp\_MAGERR_AUTO)magstat.error;phot.mag;em.opt.BdoublenullableSCgpmagIso?=- SC_gp ISO AB magnitude (SC\_gp\_MAG_ISO)magphot.mag;em.opt.Bfloatnullablee_SCgpmagIso?=- SC_gp ISO AB magnitude error (SC\_gp\_MAGERR_ISO)magstat.error;phot.mag;em.opt.BdoublenullableSCgpFlag?=- SC_gp Source Extractor internal flags (SC\_gp\_FLAGS)meta.code;phot;em.opt.BintnullableSCgpFlagIso?=- SC_gp flags: 4 means saturated pixel (s) in the isophotal area (SC\_gp\_IMAFLAGS_ISO)meta.code;phot;em.opt.BintnullableFSCVap2?=- SC_V 2 arcsec diameter aperture flux density (SC\_V\_FLUX_APER2)uJyphot.flux.density;em.opt.Vfloatnullablee_FSCVap3?=- SC_V 3 arcsec diameter aperture flux density error (SC\_Vap3)uJystat.error;phot.flux.density;em.opt.VfloatnullableFSCV?=- SC_V AUTO flux density (SC\_V\_FLUX_AUTO)uJyphot.flux.density;em.opt.Vfloatnullablee_FSCV?=- SC_V AUTO flux density error (SC\_V\_FLUXERR_AUTO)uJystat.error;phot.flux.density;em.opt.VfloatnullableSCVmagap2?=- SC_V 2 arcsec diameter aperture AB magnitude (SC\_V\_MAG_APER2)magphot.mag;em.opt.Vfloatnullablee_SCVmagap2?=- SC_V 2 arcsec diameter aperture AB magnitude error (SC\_V\_MAGERR_APER2)magstat.error;phot.mag;em.opt.VdoublenullableSCVmagap3?=- SC_V 3 arcsec diameter aperture AB magnitude (SC\_V\_MAG_APER3)magphot.mag;em.opt.Vfloatnullablee_SCVmagap3?=- SC_V 3 arcsec diameter aperture AB magnitude error (SC\_V\_MAGERR_APER3)magstat.error;phot.mag;em.opt.VdoublenullableSCVmagAuto?=- SC_V AUTO AB magnitude (SC\_V\_MAG_AUTO)magphot.mag;em.opt.Vfloatnullablee_SCVmagAuto?=- SC_V AUTO AB magnitude error (SC\_V\_MAGERR_AUTO)magstat.error;phot.mag;em.opt.VdoublenullableSCVmagIso?=- SC_V ISO AB magnitude (SC\_V\_MAG_ISO)magphot.mag;em.opt.Vfloatnullablee_SCVmagIso?=- SC_V ISO AB magnitude error (SC\_V\_MAGERR_ISO)magstat.error;phot.mag;em.opt.VdoublenullableSCVFlag?=- SC_V Source Extractor internal flags (SC\_V\_FLAGS)meta.code;phot;em.opt.VintnullableSCVFlagIso?=- SC_V flags: 4 means saturated pixel (s) in the isophotal area (SC\_V\_IMAFLAGS_ISO)meta.code;phot;em.opt.VintnullableFSCrpap2?=- SC_rp 2 arcsec diameter aperture flux density (SC\_rp\_FLUX_APER2)uJyphot.flux.density;em.opt.Rfloatnullablee_FSCrpap2?=- SC_rp 2 arcsec diameter aperture flux density error (SC\_rp\_FLUXERR_APER2)uJystat.error;phot.flux.density;em.opt.RfloatnullableFSCrpap3?=- SC_rp 3 arcsec diameter aperture flux density (SC\_rp\_FLUX_APER3)uJyphot.flux.density;em.opt.Rfloatnullablee_FSCrpap3?=- SC_rp 3 arcsec diameter aperture flux density error (SC\_rpap3)uJystat.error;phot.flux.density;em.opt.RfloatnullableFSCrp?=- SC_rp AUTO flux density (SC\_rp\_FLUX_AUTO)uJyphot.flux.density;em.opt.Rfloatnullablee_FSCrp?=- SC_rp AUTO flux density error (SC\_rp\_FLUXERR_AUTO)uJystat.error;phot.flux.density;em.opt.RfloatnullableSCrpmagap2?=- SC_rp 2 arcsec diameter aperture AB magnitude (SC\_rp\_MAG_APER2)magphot.mag;em.opt.Rfloatnullablee_SCrpmagap2?=- SC_rp 2 arcsec diameter aperture AB magnitude error (SC\_rp\_MAGERR_APER2)magstat.error;phot.mag;em.opt.RdoublenullableSCrpmagap3?=- SC_rp 3 arcsec diameter aperture AB magnitude (SC\_rp\_MAG_APER3)magphot.mag;em.opt.Rfloatnullablee_SCrpmagap3?=- SC_rp 3 arcsec diameter aperture AB magnitude error (SC\_rp\_MAGERR_APER3)magstat.error;phot.mag;em.opt.RdoublenullableSCrpmagAuto?=- SC_rp AUTO AB magnitude (SC\_rp\_MAG_AUTO)magphot.mag;em.opt.Rfloatnullablee_SCrpmagAuto?=- SC_rp AUTO AB magnitude error (SC\_rp\_MAGERR_AUTO)magstat.error;phot.mag;em.opt.RdoublenullableSCrpmagIso?=- SC_rp ISO AB magnitude (SC\_rp\_MAG_ISO)magphot.mag;em.opt.Rfloatnullablee_SCrpmagIso?=- SC_rp ISO AB magnitude error (SC\_rp\_MAGERR_ISO)magstat.error;phot.mag;em.opt.RdoublenullableSCrpFlag?=- SC_rp Source Extractor internal flags (SC\_rp\_FLAGS)meta.code;phot;em.opt.RintnullableSCrpFlagIso?=- SC_rp flags: 4 means saturated pixel (s) in the isophotal area (SC\_rp\_IMAFLAGS_ISO)meta.code;phot;em.opt.RintnullableFSCipap2?=- SC_ip 2 arcsec diameter aperture flux density (SC\_ip\_FLUX_APER2)uJyphot.flux.density;em.opt.Ifloatnullablee_FSCipap2?=- SC_ip 2 arcsec diameter aperture flux density error (SC\_ip\_FLUXERR_APER2)uJystat.error;phot.flux.density;em.opt.IfloatnullableFSCipap3?=- SC_ip 3 arcsec diameter aperture flux density (SC\_ip\_FLUX_APER3)uJyphot.flux.density;em.opt.Ifloatnullablee_FSCipap3?=- SC_ip 3 arcsec diameter aperture flux density error (SC\_ipap3)uJystat.error;phot.flux.density;em.opt.IfloatnullableFSCip?=- SC_ip AUTO flux density (SC\_ip\_FLUX_AUTO)uJyphot.flux.density;em.opt.Ifloatnullablee_FSCip?=- SC_ip AUTO flux density error (SC\_ip\_FLUXERR_AUTO)uJystat.error;phot.flux.density;em.opt.IfloatnullableSCipmagap2?=- SC_ip 2 arcsec diameter aperture AB magnitude (SC\_ip\_MAG_APER2)magphot.mag;em.opt.Ifloatnullablee_SCipmagap2?=- SC_ip 2 arcsec diameter aperture AB magnitude error (SC\_ip\_MAGERR_APER2)magstat.error;phot.mag;em.opt.IdoublenullableSCipmagap3?=- SC_ip 3 arcsec diameter aperture AB magnitude (SC\_ip\_MAG_APER3)magphot.mag;em.opt.Ifloatnullablee_SCipmagap3?=- SC_ip 3 arcsec diameter aperture AB magnitude error (SC\_ip\_MAGERR_APER3)magstat.error;phot.mag;em.opt.IdoublenullableSCipmagAuto?=- SC_ip AUTO AB magnitude (SC\_ip\_MAG_AUTO)magphot.mag;em.opt.Ifloatnullablee_SCipmagAuto?=- SC_ip AUTO AB magnitude error (SC\_ip\_MAGERR_AUTO)magstat.error;phot.mag;em.opt.IdoublenullableSCipmagIso?=- SC_ip ISO AB magnitude (SC\_ip\_MAG_ISO)magphot.mag;em.opt.Ifloatnullablee_SCipmagIso?=- SC_ip ISO AB magnitude error (SC\_ip\_MAGERR_ISO)magstat.error;phot.mag;em.opt.IdoublenullableSCipFlag?=- SC_ip Source Extractor internal flags (SC\_ip\_FLAGS)meta.code;phot;em.opt.IintnullableSCipFlagIso?=- SC_ip flags: 4 means saturated pixel (s) in the isophotal area (SC\_ip\_IMAFLAGS_ISO)meta.code;phot;em.opt.IintnullableFSCzpap2?=- SC_zp 2 arcsec diameter aperture flux density (SC\_zp\_FLUX_APER2)uJyphot.flux.density;em.opt.Ifloatnullablee_FSCzpap2?=- SC_zp 2 arcsec diameter aperture flux density error (SC\_zp\_FLUXERR_APER2)uJystat.error;phot.flux.density;em.opt.IfloatnullableFSCzpap3?=- SC_zp 3 arcsec diameter aperture flux density (SC\_zp\_FLUX_APER3)uJyphot.flux.density;em.opt.Ifloatnullablee_FSCzpap3?=- SC_zp 3 arcsec diameter aperture flux density error (SC\_zpap3)uJystat.error;phot.flux.density;em.opt.IfloatnullableFSCzp?=- SC_zp AUTO flux density (SC\_zp\_FLUX_AUTO)uJyphot.flux.density;em.opt.IfloatnullableSCzpmagap2?=- SC_zp 2 arcsec diameter aperture AB magnitude (SC\_zp\_MAG_APER2)magphot.mag;em.opt.Ifloatnullablee_SCzpmagap2?=- SC_zp 2 arcsec diameter aperture AB magnitude error (SC\_zp\_MAGERR_APER2)magstat.error;phot.mag;em.opt.IdoublenullableSCzpmagap3?=- SC_zp 3 arcsec diameter aperture AB magnitude (SC\_zp\_MAG_APER3)magphot.mag;em.opt.Ifloatnullablee_SCzpmagap3?=- SC_zp 3 arcsec diameter aperture AB magnitude error (SC\_zp\_MAGERR_APER3)magstat.error;phot.mag;em.opt.IdoublenullableSCzpmagAuto?=- SC_zp AUTO AB magnitude (SC\_zp\_MAG_AUTO)magphot.mag;em.opt.Ifloatnullablee_SCzpmagAuto?=- SC_zp AUTO AB magnitude error (SC\_zp\_MAGERR_AUTO)magstat.error;phot.mag;em.opt.IdoublenullableSCzpmagIso?=- SC_zp ISO AB magnitude (SC\_zp\_MAG_ISO)magphot.mag;em.opt.Ifloatnullablee_SCzpmagIso?=- SC_zp ISO AB magnitude error (SC\_zp\_MAGERR_ISO)magstat.error;phot.mag;em.opt.IdoublenullableSCzpFlag?=- SC_zp Source Extractor internal flags (SC\_zp\_FLAGS)meta.code;phot;em.opt.IintnullableSCzpFlagIso?=- SC_zp flags: 4 means saturated pixel (s) in the isophotal area (SC\_zp\_IMAFLAGS_ISO)meta.code;phot;em.opt.IintnullableFSCzppap2?=- SC_zpp 2 arcsec diameter aperture flux density (SC\_zpp\_FLUX_APER2)uJyphot.flux.density;em.opt.Ifloatnullablee_FSCzppap2?=- SC_zpp 2 arcsec diameter aperture flux density error (SC\_zpp\_FLUXERR_APER2)uJystat.error;phot.flux.density;em.opt.IfloatnullableFSCzppap3?=- SC_zpp 3 arcsec diameter aperture flux density (SC\_zpp\_FLUX_APER3)uJyphot.flux.density;em.opt.Ifloatnullablee_FSCzppap3?=- SC_zpp 3 arcsec diameter aperture flux density error (SC\_zppap3)uJystat.error;phot.flux.density;em.opt.IfloatnullableFSCzpp?=- SC_zpp AUTO flux density (SC\_zpp\_FLUX_AUTO)uJyphot.flux.density;em.opt.Idoublenullablee_FSCzpp?=- SC_zpp AUTO flux density error (SC\_zpp\_FLUXERR_AUTO)uJystat.error;phot.flux.density;em.opt.IfloatnullableSCzppmagap2?=- SC_zpp 2 arcsec diameter aperture AB magnitude (SC\_zpp\_MAG_APER2)magphot.mag;em.opt.Ifloatnullablee_SCzppmagap2?=- SC_zpp 2 arcsec diameter aperture AB magnitude error (SC\_zpp\_MAGERR_APER2)magstat.error;phot.mag;em.opt.IdoublenullableSCzppmagap3?=- SC_zpp 3 arcsec diameter aperture AB magnitude (SC\_zpp\_MAG_APER3)magphot.mag;em.opt.Ifloatnullablee_SCzppmagap3?=- SC_zpp 3 arcsec diameter aperture AB magnitude error (SC\_zpp\_MAGERR_APER3)magstat.error;phot.mag;em.opt.IdoublenullableSCzppmagAuto?=- SC_zpp AUTO AB magnitude (SC\_zpp\_MAG_AUTO)magphot.mag;em.opt.Ifloatnullablee_SCzppmagAuto?=- SC_zpp AUTO AB magnitude error (SC\_zpp\_MAGERR_AUTO)magstat.error;phot.mag;em.opt.IdoublenullableSCzppmagIso?=- SC_zpp ISO AB magnitude (SC\_zpp\_MAG_ISO)magphot.mag;em.opt.Ifloatnullablee_SCzppmagIso?=- SC_zpp ISO AB magnitude error (SC\_zpp\_MAGERR_ISO)magstat.error;phot.mag;em.opt.IdoublenullableSCzppFlag?=- SC_zpp Source Extractor internal flags (SC\_zpp\_FLAGS)meta.code;phot;em.opt.IintnullableSCzppFlagIso?=- SC_zpp flags: 4 means saturated pixel (s) in the isophotal area (SC\_zpp\_IMAFLAGS_ISO)meta.code;phot;em.opt.Iintnullabletotaloff2Aperture-to-total magnitude correction for 2" ap. mags, to be added (total_off2)magphot.magfloattotaloff3Aperture-to-total magnitude correction for 3" ap. mags, to be added (total_off3)magphot.magfloatFIRACCH1?=- IRAC_CH1 flux density (IRAC\_CH1\_FLUX)uJyphot.flux.density;em.IR.3-4umfloatnullablee_FIRACCH1?=- IRAC_CH1 flux density error (IRAC\_CH1\_FLUXERR)uJystat.error;phot.flux.density;em.IR.3-4umfloatnullableIRACCH1mag?=- IRAC_CH1 AB magnitude (IRAC\_CH1\_MAG)magphot.mag;em.IR.3-4umfloatnullablee_IRACCH1mag?=- IRAC_CH1 AB magnitude error (IRAC\_CH1\_MAGERR)magstat.error;phot.mag;em.IR.3-4umdoublenullableFIRACCH2?=- IRAC_CH2 flux density (IRAC\_CH2\_FLUX)uJyphot.flux.density;em.IR.4-8umfloatnullablee_FIRACCH2?=- IRAC_CH2 flux density error (IRAC\_CH2\_FLUXERR)uJystat.error;phot.flux.density;em.IR.4-8umfloatnullableIRACCH2mag?=- IRAC_CH2 AB magnitude (IRAC\_CH2\_MAG)magphot.mag;em.IR.4-8umfloatnullablee_IRACCH2mag?=- IRAC_CH2 AB magnitude error (IRAC\_CH2\_MAGERR)magstat.error;phot.mag;em.IR.4-8umdoublenullableGALEX? ID in GALEX cat. (Zamojski et al., 2007ApJS..172..468Z, Capak et al., 2007, Cat. II/284), crossm. with 0.6" rad. (ID_GALEX)meta.idintnullableFGALEXFUV?=- GALEX_FUV flux density (GALEX\_FUV\_FLUX)uJyphot.flux.density;em.UV.100-200nmfloatnullablee_FGALEXFUV[]?=- GALEX\_FUV flux density error (GALEX\_FUV\_FLUXERR)uJystat.error;phot.flux.density;em.UV.100-200nmdoublenullableGALEXFUVmag?=- GALEX_FUV AB magnitude (GALEX\_FUV\_MAG)magphot.mag;em.UV.100-200nmfloatnullablee_GALEXFUVmag?=- GALEX_FUV AB magnitude error (GALEX\_FUV\_MAGERR)magstat.error;phot.mag;em.UV.100-200nmdoublenullableFGALEXNUV?=- GALEX_NUV flux density (GALEX\_NUV\_FLUX)uJyphot.flux.density;em.UV.200-300nmfloatnullablee_FGALEXNUV[]?=- GALEX_NUV flux density error (GALEX\_NUV\_FLUXERR)uJystat.error;phot.flux.density;em.UV.200-300nmfloatnullableGALEXNUVmag?=- GALEX_NUV AB magnitude (GALEX\_NUV\_MAG)magphot.mag;em.UV.200-300nmfloatnullablee_GALEXNUVmag?=- GALEX_NUV AB magnitude error (GALEX\_NUV\_MAGERR)magstat.error;phot.mag;em.UV.200-300nmdoublenullableCOSMOS2015? ID in COSMOS2015 cat. (Laigle et al., 2016, Cat. J/ApJS/224/24) crossmatched with 0.6" radius (ID_COSMOS2015)meta.idintnullableFSPLASHCH1?=- SPLASH_CH1 flux density (SPLASH\_CH1\_FLUX)uJyphot.flux.density;em.IR.3-4umdoublenullablee_FSPLASHCH1?=- SPLASH_CH1 flux density error (SPLASH\_CH1\_FLUXERR)uJystat.error;phot.flux.density;em.IR.3-4umdoublenullableSPLASHCH1mag?=- SPLASH_CH1 AB magnitude (SPLASH\_CH1\_MAG)magphot.mag;em.IR.3-4umfloatnullablee_SPLASHCH1mag?=- SPLASH_CH1 AB magnitude error (SPLASH\_CH1\_MAGERR)magstat.error;phot.mag;em.IR.3-4umdoublenullableFSPLASHCH2?=- SPLASH_CH2 flux density (SPLASH\_CH2\_FLUX)uJyphot.flux.density;em.IR.4-8umdoublenullablee_FSPLASHCH2?=- SPLASH_CH2 flux density error (SPLASH\_CH2\_FLUXERR)uJystat.error;phot.flux.density;em.IR.4-8umdoublenullableSPLASHCH2mag?=- SPLASH_CH2 AB magnitude (SPLASH\_CH2\_MAG)magphot.mag;em.IR.4-8umfloatnullablee_SPLASHCH2mag?=- SPLASH_CH2 AB magnitude error (SPLASH\_CH2\_MAGERR)magstat.error;phot.mag;em.IR.4-8umdoublenullableFSPLASHCH3?=- SPLASH_CH3 flux density (SPLASH\_CH3\_FLUX)uJyphot.flux.density;em.IR.4-8umdoublenullablee_FSPLASHCH3?=- SPLASH_CH3 flux density error (SPLASH\_CH3\_FLUXERR)uJystat.error;phot.flux.density;em.IR.4-8umdoublenullableSPLASHCH3mag?=- SPLASH_CH3 AB magnitude (SPLASH\_CH3\_MAG)magphot.mag;em.IR.4-8umfloatnullablee_SPLASHCH3mag[]?=- SPLASH_CH3 AB magnitude error (SPLASH\_CH3\_MAGERR)magstat.error;phot.mag;em.IR.4-8umdoublenullableFSPLASHCH4?=- SPLASH_CH4 flux density (SPLASH\_CH4\_FLUX)uJyphot.flux.density;em.IR.4-8umdoublenullablee_FSPLASHCH4?=- SPLASH_CH4 flux density error (SPLASH\_CH4\_FLUXERR)uJystat.error;phot.flux.density;em.IR.4-8umfloatnullableSPLASHCH4mag?=- SPLASH_CH4 AB magnitude (SPLASH\_CH4\_MAG)magphot.mag;em.IR.4-8umfloatnullablee_SPLASHCH4mag[]?=- SPLASH_CH4 AB magnitude error (SPLASH\_CH4\_MAGERR)magstat.error;phot.mag;em.IR.4-8umdoublenullableACS? ID in HST ACS F814W cat. (Leauthaud et al., 2007ApJS..172..219L), crossm. with 0.6" radius (ID_ACS)meta.idintnullableFACSF814W?=- ACS F814W flux density (ACS\_F814W\_FLUX)uJyphot.flux.density;em.opt.Idoublenullablee_FACSF814W?=- ACS F814W flux density error (ACS\_F814W\_FLUXERR)uJystat.error;phot.flux.density;em.opt.IfloatnullableACSF814Wmag?=- ACS F814W AB magnitude (ACS\_F814W\_MAG)magphot.mag;em.opt.Ifloatnullablee_ACSF814Wmag?=- ACS F814W AB magnitude error (ACS\_F814W\_MAGERR)magstat.error;phot.mag;em.opt.IdoublenullableACSAWorld?=- ACS F814W semi-major axis length (ACS\_A_WORLD)degphys.angSize.smajAxis;em.opt.IdoublenullableACSBWorld?=- ACS F814W semi-minor axis length (ACS\_B_WORLD)degphys.angSize.sminAxis;em.opt.IdoublenullableACSthetaWorld?=- ACS F814W angle; to get PA measured from N through E, add/subtr. 90 (ACS\_THETA_WORLD)degpos.posAng;em.opt.IdoublenullableACSFWHMWorld?=- ACS F814W FWHM assuming a gaussian core (ACS\_FWHM_WORLD)degphys.angSize;em.opt.IdoublenullableACSmu?=- ACS F814W peak surface brightness above background (ACS\_MU_MAX)magphot.mag.sb;em.opt.I;stat.maxfloatnullableACSmuClass[1/3]?=- ACS F814W star/galaxy classifier: 1=galaxy, 2=star, 3=fake detection (ACS\_MU_CLASS)src.class.starGalaxy;em.opt.IintnullableCHANDRAID in Chandra cat. (Civano et al., 2016, Cat. J/ApJ/819/62, Marchesi et al., 2016, Cat. J/ApJ/817/34), crossm. w. 0.6" rad (ID_CHANDRA)meta.idcharFarmer? ID in the Farmer catalogue, crossmatched with 0.6" radius (ID_FARMER)meta.idintnullablelpzBEST?=- LePhare photo-z (=lp\_zPDF if galaxy, - if X-ray source or masked) (lp\_zBEST)src.redshift.phot;meta.maindoublenullablelptype[0/2]?=- LePhare type (0: galaxy, 1: star, 2: Xray sour., -: failure in fit) (lp\_type)src.class.starGalaxyintnullablelpzPDF?=- LePhare photo-z using the galaxy templ., median of likelihood distr. (lp\_zPDF)src.redshift.photfloatnullableb_lpzPDF?=- LePhare photo-z lower limit, 68% confidence level (galaxy templates) (lp\_zPDF\_l68)src.redshift.phot;stat.minfloatnullableB_lpzPDF?=- LePhare photo-z upper limit, 68% confidence level (galaxy templates) (lp\_zPDF\_u68)src.redshift.phot;stat.maxfloatnullablelpzMinChi2?=- LePhare photo-z using the galaxy templates, minimum chi2 (lp\_zMinChi2)src.redshift.photfloatnullablelpchi2best?=- LePhare reduced chi2 for lp\_zMinChi2 (NaN if less than 3 filters) (lp\_chi2_best)stat.fit.chi2doublenullablelpzp2?=- LePhare 2nd photo-z solution if a 2nd peak detected w. P>5% in PDF (lp\_zp_2)src.redshift.photfloatnullablelpchi22?=- LePhare reduced chi2 for the second photo-z solution (lp\_chi2_2)stat.fit.chi2doublenullablelpNbFilt?=- LePhare number of filters used in the fit (lp\_NbFilt)meta.number;instr.filterintnullablelpzq?=- LePhare photo-z for the AGN library (lp\_zq)src.redshift.photfloatnullablelpchiq?=- LePhare reduced chi2 for photo-z for the AGN library (lp\_chiq)stat.fit.chi2floatnullablelpmodq?=- LePhare best fit template number in the AGN library (lp\_modq)meta.codeintnullablelpmods?=- LePhare best fit template number in the star library (lp\_mods)meta.codeintnullableEZzphotchi2?=- EAZY chi2 at ez\_z\_phot, with z-prior (ez\_z\_phot_chi2)stat.fit.chi2doublenullablelpchis?=- LePhare reduced chi2 for the best fit with the star library (lp\_chis)stat.fit.chi2floatnullablelpmask?=- LePhare mask flag (0: in UVISTA and in clean part of HSC and SUPCAM) (lp\_mask)meta.codefloatnullablelpmodel?=- LePhare BC03 best fit template number (lp\_model)meta.codeintnullablelpage?=- LePhare BC03 age of best fit template at zPDF (lp\_age)yrtime.agedoublenullablelpdust?=- LePhare BC03 colour excess E(B-V) of best fit template at zPDF (lp\_dust)phot.color.excessfloatnullablelpAtt?=- LePhare BC03 best-fit dust law number at zPDF (lp\_Attenuation)meta.codeintnullablelpFUVMAG?=- LePhare BC03 absolute rest-frame AB mag in GALEX FUV band at zPDF (lp\_MFUV)magphys.magAbs;em.UV.100-200nmdoublenullablelpNUVMAG?=- LePhare BC03 absolute rest-frame AB mag in GALEX NUV band at zPDF (lp\_MNUV)magphys.magAbs;em.UV.200-300nmdoublenullablelpUMAG?=- LePhare BC03 absolute rest-frame AB mag in CFHT u* band at zPDF (lp\_MU)magphys.magAbs;em.opt.UdoublenullablelpGMAG?=- LePhare BC03 absolute rest-frame AB mag in Subaru/HSC g band at zPDF (lp\_MG)magphys.magAbs;em.opt.BdoublenullablelpRMAG?=- LePhare BC03 absolute rest-frame AB mag in Subaru/HSC r band at zPDF (lp\_MR)magphys.magAbs;em.opt.RdoublenullablelpIMAG?=- LePhare BC03 absolute rest-frame AB mag in Subaru/HSC i band at zPDF (lp\_MI)magphys.magAbs;em.opt.IdoublenullablelpZMAG?=- LePhare BC03 absolute rest-frame AB mag in Subaru/HSC z band at zPDF (lp\_MZ)magphys.magAbs;em.opt.IdoublenullablelpYMAG?=- LePhare BC03 absolute rest-frame AB mag in VISTA Y band at zPDF (lp\_MY)magphys.magAbs;em.IR.JdoublenullablelpJMAG?=- LePhare BC03 absolute rest-frame AB mag in VISTA J band at zPDF (lp\_MJ)magphys.magAbs;em.IR.JdoublenullablelpHMAG?=- LePhare BC03 absolute rest-frame AB mag in VISTA H band at zPDF (lp\_MH)magphys.magAbs;em.IR.HdoublenullablelpKMAG?=- LePhare BC03 absolute rest-frame AB mag in VISTA Ks band at zPDF (lp\_MK)magphys.magAbs;em.IR.KdoublenullableloglpMassmed?=- LePhare BC03 log stellar mass at zPDF (lp\_mass\_med)log(solMass)phys.massdoublenullableb_loglpMassmed?=- LePhare BC03 log stellar mass at zPDF, lower limit, 68% conf. level (lp\_mass\_med\_min68)log(solMass)phys.mass;stat.mindoublenullableB_loglpMassmed?=- LePhare BC03 log stellar mass at zPDF, upper limit, 68% conf. level (lp\_mass\_med\_max68)log(solMass)phys.mass;stat.maxdoublenullableloglpMassbest?=- LePhare BC03 log stellar mass at zMinChi2 (lp\_mass\_best)log(solMass)phys.massdoublenullableloglpSFRmed?=- LePhare BC03 log SFR at zPDF (lp\_SFR\_med)log(solMass.yr**-1)phys.SFR;stat.mindoublenullableb_loglpSFRmed?=- LePhare BC03 log SFR at zPDF, lower limit, 68% confidence level (lp\_SFR\_med\_min68)log(solMass.yr**-1)phys.SFRdoublenullableB_loglpSFRmed?=- LePhare BC03 log SFR at zPDF, upper limit, 68% confidence level (lp\_SFR\_med\_max68)log(solMass.yr**-1)phys.SFRdoublenullableloglpSFRbest?=- LePhare BC03 log SFR at zMinChi2 (lp\_SFR\_best)log(solMass.yr**-1)phys.SFRdoublenullableloglpsSFRmed?=- LePhare BC03 log sSFR at zPDF (lp\_sSFR\_med)log(yr**-1)phys.SFRdoublenullableb_loglpsSFRmed?=- LePhare BC03 log sSFR at zPDF, lower limit, 68% confidence level (lp\_sSFR\_med\_min68)log(yr**-1)phys.SFR;stat.mindoublenullableB_loglpsSFRmed?=- LePhare BC03 log sSFR at zPDF, upper limit, 68% confidence level (lp\_sSFR\_med\_max68)log(yr**-1)phys.SFR;stat.maxdoublenullableloglpsSFRbest?=- LePhare BC03 log sSFR at zMinChi2 (lp\_sSFR\_best)log(yr**-1)phys.SFRdoublenullableEZzphotrisk?=- EAZY risk parameter (Tanaka et al, 2018PASJ...70S...9T) at ez\_z\_phot, R(ez\_z_phot) (ez\_z\_phot_risk)stat.paramdoublenullableEZzminrisk?=- EAZY photo-z where risk parameter R(z) is minimised (ez\_z\_min_risk)src.redshift.photdoublenullableEZminrisk?=- EAZY risk parameter at ez\_z\_min_risk, R(ez\_z\_min_risk) (ez\_min_risk)stat.param;stat.mindoublenullableEZzrawchi2?=- EAZY photo-z where chi2 is minimised, without priors (ez\_z\_raw_chi2)src.redshift.photdoublenullableEZrawchi2?=- EAZY chi2 at ez\_z\_raw_chi2 (ez\_raw_chi2)stat.fit.chi2doublenullableEZzp025?=- EAZY 2.5% percentile of photo-z (ez\_z025)src.redshift.phot;stat.mindoublenullableEZzp160?=- EAZY 16.0% percentile of photo-z (ez\_z160)src.redshift.phot;stat.mindoublenullableEZzp500?=- EAZY 50.0% percentile of photo-z (ez\_z500)src.redshift.phot;stat.mediandoublenullableEZzp840?=- EAZY 84.0% percentile of photo-z (ez\_z840)src.redshift.phot;stat.maxdoublenullableEZnusefilt?=- EAZY no. of filters used for photo-z (only filters w/o missing data) (ez\_nusefilt)meta.number;instr.filterintnullableEZlcmin?=- EAZY minimum effective wavelength of valid filters (ez\_lc_min)0.1nmem.wl.effective;stat.mindoublenullableEZlcmax?=- EAZY minimum effective wavelength of valid filters (ez\_lc_max)0.1nmem.wl.effective;stat.maxdoublenullableEZstarminchi2?=- EAZY chi2 best stellar template fit (BT-SETTL models) as, 8% sys unc (ez\_star\_min_chi2)stat.fit.chi2doublenullableEZstarTeff?=- EAZY effective temperature of the stellar template (ez\_star_teff)Kphys.temperature.effectiveintnullableEZrestU?=- EAZY rest-frame U-band flux density (ez\_restU)uJyphot.flux.density;em.opt.Udoublenullablee_EZrestU?=- EAZY rest-frame U-band flux density uncertainty (ez\_restU\_err)uJystat.error;phot.flux.density;em.opt.UdoublenullableEZrestB?=- EAZY rest-frame B-band flux density (ez\_restB)uJyphot.flux.density;em.opt.Bdoublenullablee_EZrestB?=- EAZY rest-frame B-band flux density uncertainty (ez\_restB\_err)uJystat.error;phot.flux.density;em.opt.BdoublenullableEZrestV?=- EAZY rest-frame V-band flux density (ez\_restV)uJyphot.flux.density;em.opt.Vdoublenullablee_EZrestV?=- EAZY rest-frame V-band flux density uncertainty (ez\_restV\_err)uJystat.error;phot.flux.density;em.opt.VdoublenullableEZrestJ?=- EAZY rest-frame J-band flux density (ez\_restJ)uJyphot.flux.density;em.IR.Jdoublenullablee_EZrestJ?=- EAZY rest-frame J-band flux density uncertainty (ez\_restJ\_err)uJystat.error;phot.flux.density;em.IR.JdoublenullableEZdL?=- EAZY luminosity distance at ez\_z\_phot (ez\_dL)Mpcpos.distancedoublenullablelogEZMass?=- EAZY log stellar mass (ez\_mass)log(solMass)phys.massdoublenullablelogEZSFR?=- EAZY log SFR (ez\_sfr)log(solMass.yr**-1)phys.SFRdoublenullablelogEZsSFR?=- EAZY log sSFR (ez\_ssfr)log(yr**-1)phys.SFRdoublenullablelogEZLV?=- EAZY log V-band luminosity (ez\_Lv)log(solLum)phys.luminosity;em.opt.VdoublenullableEZLIR?=- EAZY total 8-1000um luminosity (ez\_LIR)solLumphys.luminosity;em.IRdoublenullableEZEnerAbs?=- EAZY implied absorbed energy associated with Av (ez\_energy_abs)solLumphys.energydoublenullableEZLU?=- EAZY luminosity in rest-frame U band (ez\_Lu)solLumphys.luminosity;em.opt.UdoublenullableEZLJ?=- EAZY luminosity in rest-frame J band (ez\_Lj)solLumphys.luminosity;em.IR.JdoublenullableEZL1400?=- EAZY luminosity in tophat filter at 1400{AA} (200{AA} wide) rest-frame (ez\_L1400)solLumphys.luminosity;em.UV.100-200nmdoublenullableEZL2800?=- EAZY luminosity in tophat filter at 2800{AA} (200{AA} wide) rest-frame (ez\_L2800)solLumphys.luminosity;em.UV.200-300nmdoublenullableEZLHa?=- EAZY Halpha line luminosity (reddened) (ez\_LHa)solLumphys.luminosity;em.line.HalphadoublenullableEZLOIII?=- EAZY [OIII] 4959+5007 line luminosity (reddened) (ez\_LOIII)solLumphys.luminosity;em.line.OIIIdoublenullableEZLHb?=- EAZY Hbeta line luminosity (reddened) (ez\_LHb)solLumphys.luminosity;em.line.HbetadoublenullableEZLOII?=- EAZY [OII] 3726+3729 line luminosity (reddened) (ez\_LOII)solLumphys.luminosity;em.linedoublenullableEZMLV?=- EAZY mass-to-light ratio in V band (ez\_MLv)solMass/solLumphys.composition.massLightRatio;em.opt.VdoublenullableEZAv?=- EAZY extinction in V band (ez\_Av)magphys.absorption;em.opt.VdoublenullableEZlwAgeV?=- EAZY light-weighted age in the V band (ez\_lwAgeV)Gyrtime.age;em.opt.VdoublenullablelogEZmassp025?=- EAZY 2.5% percentile of log stellar mass (ez\_mass\_p025)log(solMass)phys.mass;stat.mindoublenullablelogEZmassp160?=- EAZY 16.0% percentile of log stellar mass (ez\_mass\_p160)log(solMass)phys.mass;stat.mindoublenullablelogEZmassp500?=- EAZY 50.0% percentile of log stellar mass (ez\_mass\_p500)log(solMass)phys.mass;stat.mediandoublenullablelogEZmassp840?=- EAZY 84.0% percentile of log stellar mass (ez\_mass\_p840)log(solMass)phys.mass;stat.maxdoublenullablelogEZmassp975?=- EAZY 97.5% percentile of log stellar mass (ez\_mass\_p975)log(solMass)phys.mass;stat.maxdoublenullablelogEZsfrp025?=- EAZY 2.5% percentile of log SFR (ez\_sfr\_p025)log(solMass.yr**-1)phys.SFR;stat.mindoublenullablelogEZsfrp160?=- EAZY 16.0% percentile of log SFR (ez\_sfr\_p160)log(solMass.yr**-1)phys.SFR;stat.mindoublenullablelogEZsfrp500?=- EAZY 50.0% percentile of log SFR (ez\_sfr\_p500)log(solMass.yr**-1)phys.SFR;stat.mediandoublenullablelogEZsfrp840?=- EAZY 84.0% percentile of log SFR (ez\_sfr\_p840)log(solMass.yr**-1)phys.SFR;stat.maxdoublenullablelogEZsfrp975?=- EAZY 97.5% percentile of log SFR (ez\_sfr\_p975)log(solMass.yr**-1)phys.SFR;stat.maxdoublenullablelogEZLVp025?=- EAZY 2.5% percentile of log V-band luminosity (ez\_Lv\_p025)log(solLum)phys.luminosity;stat.min;em.opt.VdoublenullablelogEZLVp160?=- EAZY 16.0% percentile of log V-band luminosity (ez\_Lv\_p160)log(solLum)phys.luminosity;stat.min;em.opt.VdoublenullablelogEZLVp500?=- EAZY 50.0% percentile of log V-band luminosity (ez\_Lv\_p500)log(solLum)phys.luminosity;stat.median;em.opt.VdoublenullablelogEZLVp840?=- EAZY 84.0% percentile of log V-band luminosity (ez\_Lv\_p840)log(solLum)phys.luminosity;stat.max;em.opt.VdoublenullablelogEZLVp975?=- EAZY 97.5% percentile of log V-band luminosity (ez\_Lv\_p975)log(solLum)phys.luminosity;stat.max;em.opt.VdoublenullableEZLIRp025?=- EAZY 2.5% percentile of total 8-1000 um luminosity (ez\_LIR\_p025)solLumphys.luminosity;stat.min;em.IRdoublenullableEZLIRp160?=- EAZY 16.0% percentile of total 8-1000 um luminosity (ez\_LIR\_p160)solLumphys.luminosity;stat.min;em.IRdoublenullableEZLIRp500?=- EAZY 50.0% percentile of total 8-1000 um luminosity (ez\_LIR\_p500)solLumphys.luminosity;stat.median;em.IRdoublenullableEZLIRp840?=- EAZY 84.0% percentile of total 8-1000 um luminosity (ez\_LIR\_p840)solLumphys.luminosity;stat.max;em.IRdoublenullableEZLIRp975?=- EAZY 97.5% percentile of total 8-1000 um luminosity (ez\_LIR\_p975)solLumphys.luminosity;stat.max;em.IRdoublenullableEZEnerAbsp025?=- EAZY 2.5% percentile of implied absorbed energy associated with Av (ez\_energy\_abs\_p025)solLumphys.energy;stat.mindoublenullableEZEnerAbsp160?=- EAZY 16.0% percentile of implied absorbed energy associated with Av (ez\_energy\_abs\_p160)solLumphys.energy;stat.mindoublenullableEZEnerAbsp500?=- EAZY 50.0% percentile of implied absorbed energy associated with Av (ez\_energy\_abs\_p500)solLumphys.energy;stat.mediandoublenullableEZEnerAbsp840?=- EAZY 84.0% percentile of implied absorbed energy associated with Av (ez\_energy\_abs\_p840)solLumphys.energy;stat.maxdoublenullableEZEnerAbsp975?=- EAZY 97.5% percentile of implied absorbed energy associated with Av (ez\_energy\_abs\_p975)solLumphys.energy;stat.maxdoublenullableEZLUp025?=- EAZY 2.5% percentile of luminosity in rest-frame U band (ez\_Lu\_p025)solLumphys.luminosity;stat.min;em.opt.UdoublenullableEZLUp160?=- EAZY 16.0% percentile of luminosity in rest-frame U band (ez\_Lu\_p160)solLumphys.luminosity;stat.min;em.opt.UdoublenullableEZLUp500?=- EAZY 50.0% percentile of luminosity in rest-frame U band (ez\_Lu\_p500)solLumphys.luminosity;stat.median;em.opt.UdoublenullableEZLUp840?=- EAZY 84.0% percentile of luminosity in rest-frame U band (ez\_Lu\_p840)solLumphys.luminosity;stat.max;em.opt.UdoublenullableEZLUp975?=- EAZY 97.5% percentile of luminosity in rest-frame U band (ez\_Lu\_p975)solLumphys.luminosity;stat.max;em.opt.UdoublenullableEZLJp025?=- EAZY 2.5% percentile of luminosity in rest-frame J band (ez\_Lj\_p025)solLumphys.luminosity;stat.min;em.IR.JdoublenullableEZLjp160?=- EAZY 16.0% percentile of luminosity in rest-frame J band (ez\_Lj\_p160)solLumphys.luminosity;stat.min;em.IR.JdoublenullableEZLjp500?=- EAZY 50.0% percentile of luminosity in rest-frame J band (ez\_Lj\_p500)solLumphys.luminosity;stat.median;em.IR.JdoublenullableEZLJp840?=- EAZY 84.0% percentile of luminosity in rest-frame J band (ez\_Lj\_p840)solLumphys.luminosity;stat.max;em.IR.JdoublenullableEZLJp975?=- EAZY 97.5% percentile of luminosity in rest-frame J band (ez\_Lj\_p975)solLumphys.luminosity;stat.max;em.IR.JdoublenullableEZL1400p025?=- EAZY 2.5% percentile of lum tophat filter at 1400{AA} (200{AA} wide) rf (ez\_L1400\_p025)solLumphys.luminosity;stat.min;em.UV.100-200nmdoublenullableEZL1400p160?=- EAZY 16.0% percentile of lum tophat filter at 1400{AA} (200{AA} wide) rf (ez\_L1400\_p160)solLumphys.luminosity;stat.min;em.UV.100-200nmdoublenullableEZL1400p500?=- EAZY 50.0% percentile of lum tophat filter at 1400{AA} (200{AA} wide) rf (ez\_L1400\_p500)solLumphys.luminosity;stat.median;em.UV.100-200nmdoublenullableEZL1400p840?=- EAZY 84.0% percentile of lum tophat filter at 1400{AA} (200{AA} wide) rf (ez\_L1400\_p840)solLumphys.luminosity;stat.max;em.UV.100-200nmdoublenullableEZL1400p975?=- EAZY 97.5% percentile of lum tophat filter at 1400{AA} (200{AA} wide) rf (ez\_L1400\_p975)solLumphys.luminosity;stat.max;em.UV.100-200nmdoublenullableEZL2800p025?=- EAZY 2.5% percentile of lum tophat filter at 2800{AA} (200{AA} wide) rf (ez\_L2800\_p025)solLumphys.luminosity;stat.min;em.UV.200-300nmdoublenullableEZL2800p160?=- EAZY 16.0% percentile of lum tophat filter at 2800{AA} (200{AA} wide) rf (ez\_L2800\_p160)solLumphys.luminosity;stat.min;em.UV.200-300nmdoublenullableEZL2800p500?=- EAZY 50.0% percentile of lum tophat filter at 2800{AA} (200{AA} wide) rf (ez\_L2800\_p500)solLumphys.luminosity;stat.median;em.UV.200-300nmdoublenullableEZL2800p840?=- EAZY 84.0% percentile of lum tophat filter at 2800{AA} (200{AA} wide) rf (ez\_L2800\_p840)solLumphys.luminosity;stat.max;em.UV.200-300nmdoublenullableEZL2800p975?=- EAZY 97.5% percentile of lum tophat filter at 2800{AA} (200{AA} wide) rf (ez\_L2800\_p975)solLumphys.luminosity;stat.max;em.UV.200-300nmdoublenullableEZLHap025?=- EAZY 2.5% percentile of Halpha line luminosity (reddened) (ez\_LHa\_p025)solLumphys.luminosity;stat.min;em.line.HalphadoublenullableEZLHap160?=- EAZY 16.0% percentile of Halpha line luminosity (reddened) (ez\_LHa\_p160)solLumphys.luminosity;stat.min;em.line.HalphadoublenullableEZLHap500?=- EAZY 50.0% percentile of Halpha line luminosity (reddened) (ez\_LHa\_p500)solLumphys.luminosity;stat.median;em.line.HalphadoublenullableEZLHap840?=- EAZY 84.0% percentile of Halpha line luminosity (reddened) (ez\_LHa\_p840)solLumphys.luminosity;stat.max;em.line.HalphadoublenullableEZLHap975?=- EAZY 97.5% percentile of Halpha line luminosity (reddened) (ez\_LHa\_p975)solLumphys.luminosity;stat.max;em.line.HalphadoublenullableEZLOIIIp025?=- EAZY 2.5% percentile of [OIII] 4959+5007 line luminosity (reddened) (ez\_LOIII\_p025)solLumphys.luminosity;stat.min;em.line.OIIIdoublenullableEZLOIIIp160?=- EAZY 16.0% percentile of [OIII] 4959+5007 line luminosity (reddened) (ez\_LOIII\_p160)solLumphys.luminosity;stat.min;em.line.OIIIdoublenullableEZLOIIIp500?=- EAZY 50.0% percentile of [OIII] 4959+5007 line luminosity (reddened) (ez\_LOIII\_p500)solLumphys.luminosity;stat.median;em.line.OIIIdoublenullableEZLOIIIp840?=- EAZY 84.0% percentile of [OIII] 4959+5007 line luminosity (reddened) (ez\_LOIII\_p840)solLumphys.luminosity;stat.max;em.line.OIIIdoublenullableEZLOIIIp975?=- EAZY 97.5% percentile of [OIII] 4959+5007 line luminosity (reddened) (ez\_LOIII\_p975)solLumphys.luminosity;stat.max;em.line.OIIIdoublenullableEZLHbp025?=- EAZY 2.5% percentile of Hbeta line luminosity (reddened) (ez\_LHb\_p025)solLumphys.luminosity;stat.min;em.line.HbetadoublenullableEZLHbp160?=- EAZY 16.0% percentile of Hbeta line luminosity (reddened) (ez\_LHb\_p160)solLumphys.luminosity;stat.min;em.line.HbetadoublenullableEZLHbp500?=- EAZY 50.0% percentile of Hbeta line luminosity (reddened) (ez\_LHb\_p500)solLumphys.luminosity;stat.median;em.line.HbetadoublenullableEZLHbp840?=- EAZY 84.0% percentile of Hbeta line luminosity (reddened) (ez\_LHb\_p840)solLumphys.luminosity;stat.max;em.line.HbetadoublenullableEZLHbp975?=- EAZY 97.5% percentile of Hbeta line luminosity (reddened) (ez\_LHb\_p975)solLumphys.luminosity;stat.max;em.line.HbetadoublenullableEZLOIIp025?=- EAZY 2.5% percentile of [OII] 3726+3729 line luminosity (reddened) (ez\_LOII\_p025)solLumphys.luminosity;stat.min;em.linedoublenullableEZLOIIp160?=- EAZY 16.0% percentile of [OII] 3726+3729 line luminosity (reddened) (ez\_LOII\_p160)solLumphys.luminosity;stat.min;em.linedoublenullableEZLOIIp500?=- EAZY 50.0% percentile of [OII] 3726+3729 line luminosity (reddened) (ez\_LOII\_p500)solLumphys.luminosity;stat.median;em.linedoublenullableEZLOIIp840?=- EAZY 84.0% percentile of [OII] 3726+3729 line luminosity (reddened) (ez\_LOII\_p840)solLumphys.luminosity;stat.max;em.linedoublenullableEZLOIIp975?=- EAZY 97.5% percentile of [OII] 3726+3729 line luminosity (reddened) (ez\_LOII\_p975)solLumphys.luminosity;stat.max;em.linedoublenullablelogEZsSFRp025?=- EAZY 2.5% percentile of log sSFR (ez\_ssfr\_p025)log(yr**-1)phys.SFR;stat.mindoublenullablelogEZsSFRp160?=- EAZY 16.0% percentile of log sSFR (ez\_ssfr\_p160)log(yr**-1)phys.SFR;stat.mindoublenullablelogEZsSFRp500?=- EAZY 50.0% percentile of log sSFR (ez\_ssfr\_p500)log(yr**-1)phys.SFR;stat.mediandoublenullablelogEZsSFRp840?=- EAZY 84.0% percentile of log sSFR (ez\_ssfr\_p840)log(yr**-1)phys.SFR;stat.maxdoublenullablelogEZsSFRp975?=- EAZY 97.5% percentile of log sSFR (ez\_ssfr\_p975)log(yr**-1)phys.SFR;stat.maxdoublenullableEZAVp025?=- EAZY 2.5% percentile of extinction in V band (ez\_Av\_p025)magphys.absorption;stat.min;em.opt.VdoublenullableEZAVp160?=- EAZY 16.0% percentile of extinction in V band (ez\_Av\_p160)magphys.absorption;stat.min;em.opt.VdoublenullableEZAVp500?=- EAZY 50.0% percentile of extinction in V band (ez\_Av\_p500)magphys.absorption;stat.median;em.opt.VdoublenullableEZAVp840?=- EAZY 84.0% percentile of extinction in V band (ez\_Av\_p840)magphys.absorption;stat.max;em.opt.VdoublenullableEZAVp975?=- EAZY 97.5% percentile of extinction in V band (ez\_Av\_p975)magphys.absorption;stat.max;em.opt.Vdoublenullablee_FCFHTuap3? CFHT_u 3 arcsec diameter aperture flux density error (CFHT_uap3)uJystat.error;phot.flux.density;em.opt.UfloatnullableXimageObject position along X, with the scale being 0.15"/pix (X_IMAGE)pixpos.cartesian.xfloatYimageObject position along Y, with the scale being 0.15"/pix (Y_IMAGE)pixpos.cartesian.yfloatVXimageVariance of position along X (ERRX2_IMAGE)pixel**2stat.variance;pos.cartesian.xdoubleVYimageVariance of position along Y (ERRY2_IMAGE)pixel**2stat.variance;pos.cartesian.ydoubleFlagUVISTA[0/1] Flag for the UltraVISTA region (0: inside, 1: outside) (FLAG_UVISTA)meta.codeintFlagUDEEP[0/1] Flag for the UltraVISTA ultra-deep regions (0: ultra-deep, 1: deep) (FLAG_UDEEP)meta.codeintFlagCOMBINED[0/1] Comb. FLAG_UVISTA, FLAG_HSC, FLAG_SUPCAM (0: clean and inside UVISTA) (FLAG_COMBINED)meta.codeintJ/ApJS/258/11/farmerCOSMOS2020 Photometric catalogue "Farmer" created using The Farmer / The Tractor (COSMOS2020\_FARMER\_R1\_v2.2\_p3.fits) updated version, 29/03/2023SCIB427Valid[0/1] SC_IB427 flag=0 if FLUX/MAG or its error is not trustworthy (SC\_IB427_VALID)meta.code;phot;em.opt.BintIRACCH2Drift?=- IRAC_CH2 distance travelled from RA,Dec model centroid (IRAC\_CH2_DRIFT)arcsecpos.angDistance;phot;em.IR.4-8umdoublenullableIRACCH2Valid[0/1] IRAC_CH2 flag=0 if FLUX/MAG or its error is not trustworthy (IRAC\_CH2_VALID)meta.code;phot;em.IR.4-8umintFIRACCH3?=- IRAC_CH3 flux density (IRAC\_CH3_FLUX)uJyphot.flux.density;em.IR.4-8umdoublenullablee_FIRACCH3?=- IRAC_CH3 flux density error (IRAC\_CH3_FLUXERR)uJystat.error;phot.flux.density;em.IR.4-8umdoublenullableIRACCH3mag?=- IRAC_CH3 AB magnitude (IRAC\_CH3_MAG)magphot.mag;em.IR.4-8umfloatnullablee_IRACCH3mag?=- IRAC_CH3 AB magnitude error (IRAC\_CH3_MAGERR)magstat.error;phot.mag;em.IR.4-8umdoublenullableIRACCH3chi2?=- IRAC_CH3 reduced Chi2 goodness of fit stat for source prof model (IRAC\_CH3_CHISQ)stat.fit.goodness;phot;em.IR.4-8umfloatnullableIRACCH3Drift?=- IRAC_CH3 distance travelled from RA,Dec model centroid (IRAC\_CH3_DRIFT)arcsecpos.angDistance;phot;em.IR.4-8umdoublenullableIRACCH3Valid[0/1] IRAC_CH3 flag=0 if FLUX/MAG or its error is not trustworthy (IRAC\_CH3_VALID)meta.code;phot;em.IR.4-8umintFIRACCH4?=- IRAC_CH4 flux density (IRAC\_CH4_FLUX)uJyphot.flux.density;em.IR.4-8umdoublenullablee_FIRACCH4?=- IRAC_CH4 flux density error (IRAC\_CH4_FLUXERR)uJystat.error;phot.flux.density;em.IR.4-8umdoublenullableIRACCH4mag?=- IRAC_CH4 AB magnitude (IRAC\_CH4_MAG)magphot.mag;em.IR.4-8umfloatnullablee_IRACCH4mag?=- IRAC_CH4 AB magnitude error (IRAC\_CH4_MAGERR)magstat.error;phot.mag;em.IR.4-8umdoublenullableIRACCH4chi2?=- IRAC_CH4 reduced Chi2 goodness of fit stat for source prof model (IRAC\_CH4_CHISQ)stat.fit.goodness;phot;em.IR.4-8umfloatnullableIRACCH4Drift?=- IRAC_CH4 distance travelled from RA,Dec model centroid (IRAC\_CH4_DRIFT)arcsecpos.angDistance;phot;em.IR.4-8umdoublenullableIRACCH4Valid[0/1] IRAC_CH4 flag=0 if FLUX/MAG or its error is not trustworthy (IRAC\_CH4_VALID)meta.code;phot;em.IR.4-8umintFGALEXNUV?=- GALEX_NUV flux density (GALEX\_NUV_FLUX)uJyphot.flux.density;em.UV.200-300nmfloatnullablee_FGALEXNUV?=- GALEX_NUV flux density error (GALEX\_NUV_FLUXERR)uJystat.error;phot.flux.density;em.UV.200-300nmfloatnullableGALEXNUVmag?=- GALEX_NUV AB magnitude (GALEX\_NUV_MAG)magphot.mag;em.UV.200-300nmfloatnullablee_GALEXNUVmag?=- GALEX_NUV AB magnitude error (GALEX\_NUV_MAGERR)magstat.error;phot.mag;em.UV.200-300nmdoublenullableFGALEXFUV?=- GALEX_FUV flux density (GALEX\_FUV_FLUX)uJyphot.flux.density;em.UV.100-200nmfloatnullablee_FGALEXFUV?=- GALEX_FUV flux density error (GALEX\_FUV_FLUXERR)uJystat.error;phot.flux.density;em.UV.100-200nmdoublenullableClassic? ID in the Classic catalogue, crossmatched with 0.6" radius (ID_CLASSIC)meta.idintnullablelpzBEST?=- LePhare photo-z (=lp\_zPDF if galaxy, NaN if X-ray source or masked) (lp\_zBEST)src.redshift.phot;meta.maindoublenullablelptype[0/2]?=- LePhare type (0: galaxy, 1: star, 2: Xray sour., -: failure in fit) (lp\_type)src.class.starGalaxyintnullablelpzPDF?=- LePhare photo-z using the galaxy templ., median of likelihood distr. (lp\_zPDF)src.redshift.photfloatnullablelpzPDFl68?=- LePhare photo-z lower limit, 68% confidence level (galaxy templates) (lp\_zPDF_l68)src.redshift.phot;stat.minfloatnullablelpzPDFu68?=- LePhare photo-z upper limit, 68% confidence level (galaxy templates) (lp\_zPDF_u68)src.redshift.phot;stat.maxfloatnullablelpzMinChi2?=- LePhare photo-z using the galaxy templates, minimum chi2 (lp\_zMinChi2)src.redshift.photfloatnullablelpchi2best?=- LePhare reduced chi2 for lp\_zMinChi2 (NaN if less than 3 filters) (lp\_chi2_best)stat.fit.chi2doublenullablelpzp2?=- LePhare 2nd photo-z solution if a 2nd peak detected w. P>5% in PDF (lp\_zp_2)src.redshift.photfloatnullablelpchi22?=- LePhare reduced chi2 for the second photo-z solution (lp\_chi2_2)stat.fit.chi2doublenullablelpUMAG?=- LePhare BC03 absolute rest-frame AB mag in CFHT u* band at zPD (lp\_MU)magphys.magAbs;em.opt.UdoublenullablelpGMAG?=- LePhare BC03 absolute rest-frame AB mag in Subaru/HSC g band at zPDF (lp\_MG)magphys.magAbs;em.opt.BdoublenullablelpRMAG?=- LePhare BC03 absolute rest-frame AB mag in Subaru/HSC r band at zPDF (lp\_MR)magphys.magAbs;em.opt.RdoublenullablelpIMAG?=- LePhare BC03 absolute rest-frame AB mag in Subaru/HSC i band at zPDF (lp\_MI)magphys.magAbs;em.opt.IdoublenullablelpZMAG?=- LePhare BC03 absolute rest-frame AB mag in Subaru/HSC z band at zPDF (lp\_MZ)magphys.magAbs;em.opt.IdoublenullablelpYMAG?=- LePhare BC03 absolute rest-frame AB mag in Subaru/HSC Y band at zPDF (lp\_MY)magphys.magAbs;em.IR.JdoublenullablelpJMAG?=- LePhare BC03 absolute rest-frame AB mag in Subaru/HSC J band at zPDF (lp\_MJ)magphys.magAbs;em.IR.JdoublenullablelpHMAG?=- LePhare BC03 absolute rest-frame AB mag in Subaru/HSC H band at zPDF (lp\_MH)magphys.magAbs;em.IR.HdoublenullablelpKMAG?=- LePhare BC03 absolute rest-frame AB mag in Subaru/HSC Ks band at zPDF (lp\_MK)magphys.magAbs;em.IR.KdoublenullableloglpMassmed?=- LePhare BC03 log stellar mass at zPDF (lp\_mass_med)log(solMass)phys.massdoublenullableb_loglpMassmed?=- LePhare BC03 log stellar mass at zPDF, lower limit, 68% conf. level (lp\_mass\_med\_min68)log(solMass)phys.mass;stat.mindoublenullableB_loglpMassmed?=- LePhare BC03 log stellar mass at zPDF, upper limit, 68% conf. level (lp\_mass\_med\_max68)log(solMass)phys.mass;stat.maxdoublenullableloglpMassbest?=- LePhare BC03 log stellar mass at zMinChi2 (lp\_mass_best)log(solMass)phys.massdoublenullableloglpSFRbest?=- LePhare BC03 log SFR at zMinChi2 (lp\_SFR_best)log(solMass.yr**-1)phys.SFRdoublenullablelogEZSFR?=- EAZY log SFR (ez\_sfr)log(solMass.yr**-1)phys.SFRdoublenullablelogEZsSFR?=- EAZY log sSFR (ez\_ssfr)log(yr**-1)phys.SFRdoublenullablelogEZLV?=- EAZY log V-band luminosity (ez\_Lv)log(solLum)phys.luminosity;em.opt.VdoublenullableEZLIR?=- EAZY total 8-1000um luminosity (ez\_LIR)solLumphys.luminosity;em.IRdoublenullableEZEnerAbs?=- EAZY implied absorbed energy associated with Av (ez\_energy_abs)solLumphys.energydoublenullableEZLU?=- EAZY luminosity in rest-frame U band (ez\_Lu)solLumphys.luminosity;em.opt.UdoublenullableEZLJ?=- EAZY luminosity in rest-frame J band (ez\_Lj)solLumphys.luminosity;em.IR.JdoublenullableEZL1400?=- EAZY luminosity in tophat filter at 1400{AA} (200{AA} wide) rest-frame (ez\_L1400)solLumphys.luminosity;em.UV.100-200nmdoublenullableEZL2800?=- EAZY luminosity in tophat filter at 2800{AA} (200{AA} wide) rest-frame (ez\_L2800)solLumphys.luminosity;em.UV.200-300nmdoublenullableEZLHa?=- EAZY Halpha line luminosity (reddened) (ez\_LHa)solLumphys.luminosity;em.line.HalphadoublenullableEZLOIII?=- EAZY [OIII] 4959+5007 line luminosity (reddened) (ez\_LOIII)solLumphys.luminosity;em.line.OIIIdoublenullableEZLHb?=- EAZY Hbeta line luminosity (reddened) (ez\_LHb)solLumphys.luminosity;em.line.HbetadoublenullableEZLOII?=- EAZY [OII] 3726+3729 line luminosity (reddened) (ez\_LOII)solLumphys.luminosity;em.linedoublenullableEZM/LV?=- EAZY mass-to-light ratio in V band (ez\_MLv)solMass/solLumphys.composition.massLightRatio;em.opt.VdoublenullableEZAV?=- EAZY extinction in V band (ez\_Av)magphys.absorption;em.opt.VdoublenullableEZlwAgev?=- EAZY light-weighted age in the V band (ez\_lwAgeV)Gyrtime.age;em.opt.VdoublenullablelogEZMassp025?=- EAZY 2.5% percentile of log stellar mass (ez\_mass_p025)log(solMass)phys.mass;stat.mindoublenullableFarmerIDFarmer internal source identifier ({brick}_{source}) (FARMER_ID)meta.idcharFUVISTAY?=- UVISTA_Y flux density (UVISTA\_Y_FLUX)uJyphot.flux.density;em.IR.JdoublenullableCFHTustarmag?=- CFHT_ustar AB magnitude (CFHT\_ustar_MAG)magphot.mag;em.opt.Ufloatnullablee_FCFHTu?=- CFHT_u flux density error (CFHT\_u_FLUXERR)uJystat.error;phot.flux.density;em.opt.UdoublenullableFHSCz?=- HSC_i flux density (HSC\_z_FLUX)uJyphot.flux.density;em.opt.Idoublenullablee_CFHTustarmag?=- CFHT_ustar AB magnitude error (CFHT\_ustar_MAGERR)magstat.error;phot.mag;em.opt.UdoublenullableCFHTumag?=- CFHT_u AB magnitude (CFHT\_u_MAG)magphot.mag;em.opt.UfloatnullableHSCiValid[0/1] HSC\_i flag=0 if FLUX/MAG or its error is not trustworthy (HSC\_i_VALID)meta.code;phot;em.opt.IintrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNGroup? Farmer group occupation number (N_GROUP)meta.numberintnullableFModel[0/2]? Flag (0: OK, 1: failed to converge, 2: drifted >0.6" from detection) (MODEL_FLAG)meta.codeintnullableFCFHTu?=- CFHT_u flux density (CFHT\_u_FLUX)uJyphot.flux.density;em.opt.Udoublenullablee_CFHTumag?=- CFHT_u AB magnitude error (CFHT\_u_MAGERR)magstat.error;phot.mag;em.opt.UdoublenullableCFHTuchi2?=- CFHT_u reduced Chi2 goodness of fit stat for source prof model (CFHT\_u_CHISQ)stat.fit.goodness;phot;em.opt.UfloatnullableCFHTuDrift?=- CFHT_u distance travelled from RA,Dec model centroid (CFHT\_u_DRIFT)arcsecpos.angDistance;phot;em.opt.UdoublenullableFCFHTustar?=- CFHT_ustar flux density (CFHT\_ustar_FLUX)uJyphot.flux.density;em.opt.Udoublenullablee_FCFHTustar?=- CFHT_ustar flux density error (CFHT\_ustar_FLUXERR)uJystat.error;phot.flux.density;em.opt.UdoublenullableCFHTustarchi2?=- CFHT_ustar reduced Chi2 goodness of fit stat for source prof model (CFHT\_ustar_CHISQ)stat.fit.goodness;phot;em.opt.UfloatnullableCFHTustarDrift?=- CFHT_ustar distance travelled from RA,Dec model centroid (CFHT\_ustar_DRIFT)arcsecpos.angDistance;phot;em.opt.UdoublenullableFHSCg?=- HSC\_g flux density (HSC\_g_FLUX)uJyphot.flux.density;em.opt.Bdoublenullablee_FHSCg?=- HSC\_g flux density error (HSC\_g_FLUXERR)uJystat.error;phot.flux.density;em.opt.BdoublenullableHSCgmag?=- HSC_g AB magnitude (HSC\_g_MAG)magphot.mag;em.opt.Bfloatnullablee_HSCgmag?=- HSC_g AB magnitude error (HSC\_g_MAGERR)magstat.error;phot.mag;em.opt.BdoublenullableHSCgchi2?=- HSC_g reduced Chi2 goodness of fit stat for source prof model (HSC\_g_CHISQ)stat.fit.goodness;phot;em.opt.BdoublenullableHSCgDrift?=- HSC_g distance travelled from RA,Dec model centroid (HSC\_g_DRIFT)arcsecpos.angDistance;phot;em.opt.BdoublenullableFHSCr?=- HSC_r flux density (HSC\_r_FLUX)uJyphot.flux.density;em.opt.Rdoublenullablee_FHSCr?=- HSC_r flux density error (HSC\_r_FLUXERR)uJystat.error;phot.flux.density;em.opt.RdoublenullableHSCrmag?=- HSC_r AB magnitude (HSC\_r_MAG)magphot.mag;em.opt.Rfloatnullablee_HSCrmag?=- HSC_r AB magnitude error (HSC\_r_MAGERR)magstat.error;phot.mag;em.opt.RdoublenullableHSCrchi2?=- HSC_r reduced Chi2 goodness of fit stat for source prof model (HSC\_r_CHISQ)stat.fit.goodness;phot;em.opt.RdoublenullableHSCrDrift?=- HSC_r distance travelled from RA,Dec model centroid (HSC\_r_DRIFT)arcsecpos.angDistance;phot;em.opt.RdoublenullableFHSCi?=- HSC_i flux density (HSC\_i_FLUX)uJyphot.flux.density;em.opt.Idoublenullablee_FHSCi?=- HSC_i flux density error (HSC\_i_FLUXERR)uJystat.error;phot.flux.density;em.opt.IdoublenullableHSCimag?=- HSC_i AB magnitude (HSC\_i_MAG)magphot.mag;em.opt.Ifloatnullablee_HSCimag?=- HSC_i AB magnitude error (HSC\_i_MAGERR)magstat.error;phot.mag;em.opt.IdoublenullableHSCichi2?=- HSC_i reduced Chi2 goodness of fit stat for source prof model (HSC\_i_CHISQ)stat.fit.goodness;phot;em.opt.IdoublenullableHSCiDrift?=- HSC_i distance travelled from RA,Dec model centroid (HSC\_i_DRIFT)arcsecpos.angDistance;phot;em.opt.Idoublenullablee_FHSCz?=- HSC_z flux density error (HSC\_z_FLUXERR)uJystat.error;phot.flux.density;em.opt.IdoublenullableHSCzmag?=- HSC_z AB magnitude (HSC\_z_MAG)magphot.mag;em.opt.Ifloatnullablee_HSCzmag?=- HSC_z AB magnitude error (HSC\_z_MAGERR)magstat.error;phot.mag;em.opt.IdoublenullableHSCzchi2?=- HSC_z reduced Chi2 goodness of fit stat for source prof model (HSC\_z_CHISQ)stat.fit.goodness;phot;em.opt.IdoublenullableHSCzDrift?=- HSC_z distance travelled from RA,Dec model centroid (HSC\_z_DRIFT)arcsecpos.angDistance;phot;em.opt.IdoublenullableFHSCy?=- HSC_y flux density (HSC\_y_FLUX)uJyphot.flux.density;em.opt.Idoublenullablee_FHSCy?=- HSC_y flux density error (HSC\_y_FLUXERR)uJystat.error;phot.flux.density;em.opt.IdoublenullableHSCymag?=- HSC_y AB magnitude (HSC\_y_MAG)magphot.mag;em.opt.Ifloatnullablee_HSCymag?=- HSC_y AB magnitude error (HSC\_y_MAGERR)magstat.error;phot.mag;em.opt.IdoublenullableHSCychi2?=- HSC_y reduced Chi2 goodness of fit stat for source prof model (HSC\_y_CHISQ)stat.fit.goodness;phot;em.opt.IfloatnullableHSCyDrift?=- HSC_y distance travelled from RA,Dec model centroid (HSC\_y_DRIFT)arcsecpos.angDistance;phot;em.opt.IdoublenullableHSCyValid[0/1] HSC_y flag=0 if FLUX/MAG or its error is not trustworthy (HSC\_y_VALID)meta.code;phot;em.opt.Iinte_FUVISTAY?=- UVISTA_Y flux density error (UVISTA\_Y_FLUXERR)uJystat.error;phot.flux.density;em.IR.JdoublenullableUVISTAYmag?=- UVISTA_Y AB magnitude (UVISTA\_Y_MAG)magphot.mag;em.IR.Jfloatnullablee_UVISTAYmag?=- UVISTA_Y AB magnitude error (UVISTA\_Y_MAGERR)magstat.error;phot.mag;em.IR.JdoublenullableUVISTAYchi2?=- UVISTA_Y reduced Chi2 goodness of fit stat for source prof model (UVISTA\_Y_CHISQ)stat.fit.goodness;phot;em.IR.JdoublenullableUVISTAYDrift?=- UVISTA_Y distance travelled from RA,Dec model centroid (UVISTA\_Y_DRIFT)arcsecpos.angDistance;phot;em.IR.JdoublenullableUVISTAYValid[0/1] UVISTA_Y flag=0 if FLUX/MAG or its error is not trustworthy (UVISTA\_Y_VALID)meta.code;phot;em.IR.JintFUVISTAJ?=- UVISTA_J flux density (UVISTA\_J_FLUX)uJyphot.flux.density;em.IR.Jdoublenullablee_FUVISTAJ?=- UVISTA_J flux density error (UVISTA\_J_FLUXERR)uJystat.error;phot.flux.density;em.IR.JdoublenullableUVISTAJmag?=- UVISTA_J AB magnitude (UVISTA\_J_MAG)magphot.mag;em.IR.Jfloatnullablee_UVISTAJmag?=- UVISTA_J AB magnitude error (UVISTA\_J_MAGERR)magstat.error;phot.mag;em.IR.JdoublenullableUVISTAJchi2?=- UVISTA_J reduced Chi2 goodness of fit stat for source prof model (UVISTA\_J_CHISQ)stat.fit.goodness;phot;em.IR.JdoublenullableUVISTAJDrift?=- UVISTA_J distance travelled from RA,Dec model centroid (UVISTA\_J_DRIFT)arcsecpos.angDistance;phot;em.IR.JdoublenullableUVISTAJValid[0/1] UVISTA_J flag=0 if FLUX/MAG or its error is not trustworthy (UVISTA\_J_VALID)meta.code;phot;em.IR.JintFUVISTAH?=- UVISTA_H flux density (UVISTA\_H_FLUX)uJyphot.flux.density;em.IR.Hdoublenullablee_FUVISTAH?=- UVISTA_H flux density error (UVISTA\_H_FLUXERR)uJystat.error;phot.flux.density;em.IR.HdoublenullableUVISTAHmag?=- UVISTA_H AB magnitude (UVISTA\_H_MAG)magphot.mag;em.IR.Hfloatnullablee_UVISTAHmag?=- UVISTA_H AB magnitude error (UVISTA\_H_MAGERR)magstat.error;phot.mag;em.IR.HdoublenullableUVISTAHchi2?=- UVISTA_H reduced Chi2 goodness of fit stat for source prof model (UVISTA\_H_CHISQ)stat.fit.goodness;phot;em.IR.HdoublenullableUVISTAHDrift?=- UVISTA_H distance travelled from RA,Dec model centroid (UVISTA\_H_DRIFT)arcsecpos.angDistance;phot;em.IR.HdoublenullableUVISTAHValid[0/1] UVISTA_H flag=0 if FLUX/MAG or its error is not trustworthy (UVISTA\_H_VALID)meta.code;phot;em.IR.HintFUVISTAKs?=- UVISTA_Ks flux density (UVISTA\_Ks_FLUX)uJyphot.flux.density;em.IR.Kdoublenullablee_FUVISTAKs?=- UVISTA_Ks flux density error (UVISTA\_Ks_FLUXERR)uJystat.error;phot.flux.density;em.IR.KdoublenullableUVISTAKsmag?=- UVISTA_Ks AB magnitude (UVISTA\_Ks_MAG)magphot.mag;em.IR.Kfloatnullablee_UVISTAKsmag?=- UVISTA_Ks AB magnitude error (UVISTA\_Ks_MAGERR)magstat.error;phot.mag;em.IR.KdoublenullableFSCIA738?=- SC_IA738 flux density (SC\_IA738_FLUX)uJyphot.flux.density;em.opt.RdoublenullableUVISTAKschi2?=- UVISTA_Ks reduced Chi2 goodness of fit stat for source prof model (UVISTA\_Ks_CHISQ)stat.fit.goodness;phot;em.IR.KdoublenullableUVISTAKsDrift?=- UVISTA_Ks distance travelled from RA,Dec model centroid (UVISTA\_Ks_DRIFT)arcsecpos.angDistance;phot;em.IR.KdoublenullableUVISTAKsValid[0/1] UVISTA_Ks flag=0 if FLUX/MAG or its error is not trustworthy (UVISTA\_Ks_VALID)meta.code;phot;em.IR.KintFUVISTANB118?=- UVISTA_NB118 flux density (UVISTA\_NB118_FLUX)uJyphot.flux.density;em.IR.Jdoublenullablee_FUVISTANB118?=- UVISTA_NB118 flux density error (UVISTA\_NB118_FLUXERR)uJystat.error;phot.flux.density;em.IR.JdoublenullableUVISTANB118mag?=- UVISTA_NB118 AB magnitude (UVISTA\_NB118_MAG)magphot.mag;em.IR.Jfloatnullablee_UVISTANB118mag?=- UVISTA_NB118 AB magnitude error (UVISTA\_NB118_MAGERR)magstat.error;phot.mag;em.IR.JdoublenullableUVISTANB118chi2?=- UVISTA_NB118 reduced Chi2 goodness of fit stat for source prof model (UVISTA\_NB118_CHISQ)stat.fit.goodness;phot;em.IR.JfloatnullableUVISTANB118Drift?=- UVISTA_NB118 distance travelled from RA,Dec model centroid (UVISTA\_NB118_DRIFT)arcsecpos.angDistancedoublenullableUVISTANB118Valid[0/1] UVISTA_NB118 flag=0 if FLUX/MAG or its error is not trustworthy (UVISTA\_NB118_VALID)meta.codeintFSCIB427?=- SC_IB427 flux density (SC\_IB427_FLUX)uJyphot.flux.density;em.opt.Bdoublenullablee_FSCIB427?=- SC_IB427 flux density error (SC\_IB427_FLUXERR)uJystat.error;phot.flux.density;em.opt.BdoublenullableSCIB427mag?=- SC_IB427 AB magnitude (SC\_IB427_MAG)magphot.mag;em.opt.Bfloatnullablee_SCIB427mag?=- SC_IB427 AB magnitude error (SC\_IB427_MAGERR)magstat.error;phot.mag;em.opt.BdoublenullableSCIB427chi2?=- SC_IB427 reduced Chi2 goodness of fit stat for source prof model (SC\_IB427_CHISQ)stat.fit.goodness;phot;em.opt.BfloatnullableSCIB427Drift?=- SC_IB427 distance travelled from RA,Dec model centroid (SC\_IB427_DRIFT)arcsecpos.angDistance;phot;em.opt.BdoublenullableFSCIB464?=- SC_IB464 flux density (SC\_IB464_FLUX)uJyphot.flux.density;em.opt.Bdoublenullablee_FSCIB464?=- SC_IB464 flux density error (SC\_IB464_FLUXERR)uJystat.error;phot.flux.density;em.opt.BdoublenullableSCIB464mag?=- SC_IB464 AB magnitude (SC\_IB464_MAG)magphot.mag;em.opt.Bfloatnullablee_SCIB464mag?=- SC_IB464 AB magnitude error (SC\_IB464_MAGERR)magstat.error;phot.mag;em.opt.BdoublenullableSCIB464chi2?=- SC_IB464 reduced Chi2 goodness of fit stat for source prof model (SC\_IB464_CHISQ)stat.fit.goodness;phot;em.opt.BfloatnullableSCIB464Drift?=- SC_IB464 distance travelled from RA,Dec model centroid (SC\_IB464_DRIFT)arcsecpos.angDistance;phot;em.opt.BdoublenullableSCIB464Valid[0/1] SC_IB464 flag=0 if FLUX/MAG or its error is not trustworthy (SC\_IB464_VALID)meta.code;phot;em.opt.BintFSCIA484?=- SC_IA484 flux density (SC\_IA484_FLUX)uJyphot.flux.density;em.opt.Bdoublenullablee_FSCIA484?=- SC_IA484 flux density error (SC\_IA484_FLUXERR)uJystat.error;phot.flux.density;em.opt.BdoublenullableSCIA484mag?=- SC_IA484 AB magnitude (SC\_IA484_MAG)magphot.mag;em.opt.Bfloatnullablee_SCIA484mag?=- SC_IA484 AB magnitude error (SC\_IA484_MAGERR)magstat.error;phot.mag;em.opt.BdoublenullableSCIA484chi2?=- SC_IA484 reduced Chi2 goodness of fit stat for source prof model (SC\_IA484_CHISQ)stat.fit.goodness;phot;em.opt.BfloatnullableSCIA484Drift?=- SC_IA484 distance travelled from RA,Dec model centroid (SC\_IA484_DRIFT)arcsecpos.angDistance;phot;em.opt.BdoublenullableSCIA484Valid[0/1] SC_IA484 flag=0 if FLUX/MAG or its error is not trustworthy (SC\_IA484_VALID)meta.code;phot;em.opt.BintFSCIB505?=- SC_IB505 flux density (SC\_IB505_FLUX)uJyphot.flux.density;em.opt.Vdoublenullablee_FSCIB505?=- SC_IB505 flux density error (SC\_IB505_FLUXERR)uJystat.error;phot.flux.density;em.opt.VdoublenullableSCIB505mag?=- SC_IB505 AB magnitude (SC\_IB505_MAG)magphot.mag;em.opt.Vfloatnullablee_SCIB505mag?=- SC_IB505 AB magnitude error (SC\_IB505_MAGERR)magstat.error;phot.mag;em.opt.VdoublenullableSCIB505chi2?=- SC_IB505 reduced Chi2 goodness of fit stat for source prof model (SC\_IB505_CHISQ)stat.fit.goodness;phot;em.opt.VfloatnullableIRACCH1Valid[0/1] IRAC_CH1 flag=0 if FLUX/MAG or its error is not trustworthy (IRAC\_CH1_VALID)meta.code;phot;em.IR.3-4umintSCIB505Drift?=- SC_IB505 distance travelled from RA,Dec model centroid (SC\_IB505_DRIFT)arcsecpos.angDistance;phot;em.opt.VdoublenullableSCIB505Valid[0/1] SC_IB505 flag=0 if FLUX/MAG or its error is not trustworthy (SC\_IB505_VALID)meta.code;phot;em.opt.VintFSCIA527?=- SC_IA527 flux density (SC\_IA527_FLUX)uJyphot.flux.density;em.opt.Vdoublenullablee_FSCIA527?=- SC_IA527 flux density error (SC\_IA527_FLUXERR)uJystat.error;phot.flux.density;em.opt.VdoublenullableSCIA527mag?=- SC_IA527 AB magnitude (SC\_IA527_MAG)magphot.mag;em.opt.Vdoublenullablee_SCIA527mag?=- SC_IA527 AB magnitude error (SC\_IA527_MAGERR)magstat.error;phot.mag;em.opt.VdoublenullableSCIA527chi2?=- SC_IA527 reduced Chi2 goodness of fit stat for source prof model (SC\_IA527_CHISQ)stat.fit.goodness;phot;em.opt.VdoublenullableSCIA527Drift?=- SC_IA527 distance travelled from RA,Dec model centroid (SC\_IA527_DRIFT)arcsecpos.angDistance;phot;em.opt.VdoublenullableSCIA527Valid[0/1] SC_IA527 flag=0 if FLUX/MAG or its error is not trustworthy (SC\_IA527_VALID)meta.code;phot;em.opt.VintFSCIB574?=- SC_IB574 flux density (SC\_IB574_FLUX)uJyphot.flux.density;em.opt.Vdoublenullablee_FSCIB574?=- SC_IB574 flux density error (SC\_IB574_FLUXERR)uJystat.error;phot.flux.density;em.opt.VdoublenullableSCIB574mag?=- SC_IB574 AB magnitude (SC\_IB574_MAG)magphot.mag;em.opt.Vfloatnullablee_SCIB574mag?=- SC_IB574 AB magnitude error (SC\_IB574_MAGERR)magstat.error;phot.mag;em.opt.VdoublenullableSCIB574chi2?=- SC_IB574 reduced Chi2 goodness of fit stat for source prof model (SC\_IB574_CHISQ)stat.fit.goodness;phot;em.opt.VfloatnullableSCIB574Drift?=- SC_IB574 distance travelled from RA,Dec model centroid (SC\_IB574_DRIFT)arcsecpos.angDistance;phot;em.opt.VdoublenullableSCIB574Valid[0/1] SC_IB574 flag=0 if FLUX/MAG or its error is not trustworthy (SC\_IB574_VALID)meta.code;phot;em.opt.VintFSCIA624?=- SC_IA624 flux density (SC\_IA624_FLUX)uJyphot.flux.density;em.opt.Rdoublenullablee_FSCIA624?=- SC_IA624 flux density error (SC\_IA624_FLUXERR)uJystat.error;phot.flux.density;em.opt.RdoublenullableSCIA624mag?=- SC_IA624 AB magnitude (SC\_IA624_MAG)magphot.mag;em.opt.Rdoublenullablee_SCIA624mag?=- SC_IA624 AB magnitude error (SC\_IA624_MAGERR)magstat.error;phot.mag;em.opt.RdoublenullableSCIA624chi2?=- SC_IA624 reduced Chi2 goodness of fit stat for source prof model (SC\_IA624_CHISQ)stat.fit.goodness;phot;em.opt.RdoublenullableSCIA624Drift?=- SC_IA624 distance travelled from RA,Dec model centroid (SC\_IA624_DRIFT)arcsecpos.angDistance;phot;em.opt.RdoublenullableSCIA624Valid[0/1] SC_IA624 flag=0 if FLUX/MAG or its error is not trustworthy (SC\_IA624_VALID)meta.code;phot;em.opt.RintFSCIA679?=- SC_IA679 flux density (SC\_IA679_FLUX)uJyphot.flux.density;em.opt.Rdoublenullablee_FSCIA679?=- SC_IA679 flux density error (SC\_IA679_FLUXERR)uJystat.error;phot.flux.density;em.opt.RdoublenullableSCIA679mag?=- SC_IA679 AB magnitude (SC\_IA679_MAG)magphot.mag;em.opt.Rfloatnullablee_SCIA679mag?=- SC_IA679 AB magnitude error (SC\_IA679_MAGERR)magstat.error;phot.mag;em.opt.RdoublenullableSCIA679chi2?=- SC_IA679 reduced Chi2 goodness of fit stat for source prof model (SC\_IA679_CHISQ)stat.fit.goodness;phot;em.opt.RfloatnullableSCIA679Drift?=- SC_IA679 distance travelled from RA,Dec model centroid (SC\_IA679_DRIFT)arcsecpos.angDistance;phot;em.opt.RdoublenullableSCIA679Valid[0/1] SC_IA679 flag=0 if FLUX/MAG or its error is not trustworthy (SC\_IA679_VALID)meta.code;phot;em.opt.RintFSCIB709?=- SC_IB709 flux density (SC\_IB709_FLUX)uJyphot.flux.density;em.opt.Rdoublenullablee_FSCIB709?=- SC_IB709 flux density error (SC\_IB709_FLUXERR)uJystat.error;phot.flux.density;em.opt.RdoublenullableSCIB709mag?=- SC_IB709 AB magnitude (SC\_IB709_MAG)magphot.mag;em.opt.Rfloatnullablee_SCIB709mag?=- SC_IB709 AB magnitude error (SC\_IB709_MAGERR)magstat.error;phot.mag;em.opt.RdoublenullableSCIB709chi2?=- SC_IB709 reduced Chi2 goodness of fit stat for source prof model (SC\_IB709_CHISQ)stat.fit.goodness;phot;em.opt.RfloatnullableSCIB709Drift?=- SC_IB709 distance travelled from RA,Dec model centroid (SC\_IB709_DRIFT)arcsecpos.angDistance;phot;em.opt.RdoublenullableSCIB709Valid[0/1] SC_IB709_VALID flag=0 if FLUX/MAG or its error is not trustworthy (SC\_IB709_VALID)meta.code;phot;em.opt.Rinte_FSCIA738?=- SC_IA738 flux density error (SC\_IA738_FLUXERR)uJystat.error;phot.flux.density;em.opt.RdoublenullableSCIA738mag?=- SC_IA738 AB magnitude (SC\_IA738_MAG)magphot.mag;em.opt.Rfloatnullablee_SCIA738mag?=- SC_IA738 AB magnitude error (SC\_IA738_MAGERR)magstat.error;phot.mag;em.opt.RdoublenullableSCIA738chi2?=- SC_IA738 reduced Chi2 goodness of fit stat for source prof model (SC\_IA738_CHISQ)stat.fit.goodness;phot;em.opt.RfloatnullableSCIA738Drift?=- SC_IA738 distance travelled from RA,Dec model centroid (SC\_IA738_DRIFT)arcsecpos.angDistance;phot;em.opt.RdoublenullableFSCIA767?=- SC_IA767 flux density (SC\_IA767_FLUX)uJyphot.flux.density;em.opt.Idoublenullablee_FSCIA767?=- SC_IA767 flux density error (SC\_IA767_FLUXERR)uJystat.error;phot.flux.density;em.opt.IdoublenullableSCIA767mag?=- SC_IA767 AB magnitude (SC\_IA767_MAG)magphot.mag;em.opt.Ifloatnullablee_SCIA767mag?=- SC_IA767 AB magnitude error (SC\_IA767_MAGERR)magstat.error;phot.mag;em.opt.IdoublenullableSCIA767chi2?=- SC_IA767 reduced Chi2 goodness of fit stat for source prof model (SC\_IA767_CHISQ)stat.fit.goodness;phot;em.opt.IfloatnullableSCIA767Drift?=- SC_IA767 distance travelled from RA,Dec model centroid (SC\_IA767_DRIFT)arcsecpos.angDistance;phot;em.opt.IdoublenullableFSCIB827?=- SC_IB827 flux density (SC\_IB827_FLUX)uJyphot.flux.density;em.opt.Idoublenullablee_FSCIB827?=- SC_IB827 flux density error (SC\_IB827_FLUXERR)uJystat.error;phot.flux.density;em.opt.IdoublenullableSCIB827mag?=- SC_IB827 AB magnitude (SC\_IB827_MAG)magphot.mag;em.opt.Ifloatnullablee_SCIB827mag?=- SC_IB827 AB magnitude error (SC\_IB827_MAGERR)magstat.error;phot.mag;em.opt.IdoublenullableSCIB827chi2?=- SC_IB827 reduced Chi2 goodness of fit stat for source prof model (SC\_IB827_CHISQ)stat.fit.goodness;phot;em.opt.IfloatnullableSCIB827Drift?=- SC_IB827 distance travelled from RA,Dec model centroid (SC\_IB827_DRIFT)arcsecpos.angDistance;phot;em.opt.IdoublenullableFSCNB711?=- SC_NB711 flux density (SC\_NB711_FLUX)uJyphot.flux.density;em.opt.Rdoublenullablee_FSCNB711?=- SC_NB711 flux density error (SC\_NB711_FLUXERR)uJystat.error;phot.flux.density;em.opt.RdoublenullableSCNB711mag?=- SC_NB711 AB magnitude (SC\_NB711_MAG)magphot.mag;em.opt.Rfloatnullablee_SCNB711mag?=- SC_NB711 AB magnitude error (SC\_NB711_MAGERR)magstat.error;phot.mag;em.opt.RdoublenullableSCNB711chi2?=- SC_NB711 reduced Chi2 goodness of fit stat for source prof model (SC\_NB711_CHISQ)stat.fit.goodness;phot;em.opt.RfloatnullableSCNB711Drift?=- SC_NB711 distance travelled from RA,Dec model centroid (SC\_NB711_DRIFT)arcsecpos.angDistance;phot;em.opt.RdoublenullableFSCNB816?=- SC_NB816 flux density (SC\_NB816_FLUX)uJyphot.flux.density;em.opt.Idoublenullablee_FSCNB816?=- SC_NB816 flux density error (SC\_NB816_FLUXERR)uJystat.error;phot.flux.density;em.opt.IdoublenullableSCNB816mag?=- SC_NB816 AB magnitude (SC\_NB816_MAG)magphot.mag;em.opt.Ifloatnullablee_SCNB816mag?=- SC_NB816 AB magnitude error (SC\_NB816_MAGERR)magstat.error;phot.mag;em.opt.IdoublenullableSCNB816chi2?=- SC_NB816 reduced Chi2 goodness of fit stat for source prof model (SC\_NB816_CHISQ)stat.fit.goodness;phot;em.opt.IfloatnullableSCNB816Drift?=- SC_NB816 distance travelled from RA,Dec model centroid (SC\_NB816_DRIFT)arcsecpos.angDistance;phot;em.opt.IdoublenullableSCNB816Valid[0/1] SC_NB816 flag=0 if FLUX/MAG or its error is not trustworthy (SC\_NB816_VALID)meta.code;phot;em.opt.IintFIRACCH1?=- IRAC_CH1 flux density (IRAC\_CH1_FLUX)uJyphot.flux.density;em.IR.3-4umdoublenullablee_FIRACCH1?=- IRAC_CH1 flux density error (IRAC\_CH1_FLUXERR)uJystat.error;phot.flux.density;em.IR.3-4umdoublenullableIRACCH1mag?=- IRAC_CH1 AB magnitude (IRAC\_CH1_MAG)magphot.mag;em.IR.3-4umfloatnullablee_IRACCH1mag?=- IRAC_CH1 AB magnitude error (IRAC\_CH1_MAGERR)magstat.error;phot.mag;em.IR.3-4umdoublenullableIRACCH1chi2?=- IRAC_CH1 reduced Chi2 goodness of fit stat for source prof model (IRAC\_CH1_CHISQ)stat.fit.goodness;phot;em.IR.3-4umdoublenullableIRACCH1Drift?=- IRAC_CH1 distance travelled from RA,Dec model centroid (IRAC\_CH1_DRIFT)arcsecpos.angDistance;phot;em.IR.3-4umdoublenullableFIRACCH2?=- IRAC_CH2 flux density (IRAC\_CH2_FLUX)uJyphot.flux.density;em.IR.4-8umdoublenullablee_FIRACCH2?=- IRAC_CH2 flux density error (IRAC\_CH2_FLUXERR)uJystat.error;phot.flux.density;em.IR.4-8umdoublenullableIRACCH2mag?=- IRAC_CH2 AB magnitude (IRAC\_CH2_MAG)magphot.mag;em.IR.4-8umfloatnullablee_IRACCH2mag?=- IRAC_CH2 AB magnitude error (IRAC\_CH2_MAGERR)magstat.error;phot.mag;em.IR.4-8umdoublenullableIRACCH2chi2?=- IRAC_CH2 reduced Chi2 goodness of fit stat for source prof model (IRAC\_CH2_CHISQ)stat.fit.goodness;phot;em.IR.4-8umfloatnullableGALEX? ID in GALEX cat. (Zamojski et al., 2007ApJS..172..468Z, Capak et al., 2007, Cat. II/284), crossm. with 0.6" rad. (ID_GALEX)meta.idintnullableGALEXFUVmag?=- GALEX_FUV AB magnitude (GALEX\_FUV_MAG)magphot.mag;em.UV.100-200nmfloatnullablee_GALEXFUVmag?=- GALEX_FUV AB magnitude error (GALEX\_FUV_MAGERR)magstat.error;phot.mag;em.UV.100-200nmdoublenullableFSPLASHCH1?=- SPLASH_CH1 flux density (SPLASH\_CH1_FLUX)uJyphot.flux.density;em.IR.3-4umfloatnullablee_FSPLASHCH1?=- SPLASH_CH1 flux density error (SPLASH\_CH1_FLUXERR)uJystat.error;phot.flux.density;em.IR.3-4umfloatnullableSPLASHCH1mag?=- SPLASH_CH1 AB magnitude (SPLASH\_CH1_MAG)magphot.mag;em.IR.3-4umfloatnullablee_SPLASHCH1mag?=- SPLASH_CH1 AB magnitude error (SPLASH\_CH1_MAGERR)magstat.error;phot.mag;em.IR.3-4umdoublenullableFSPLASHCH2?=- SPLASH_CH2 flux density (SPLASH\_CH2_FLUX)uJyphot.flux.density;em.IR.4-8umfloatnullablee_FSPLASHCH2?=- SPLASH_CH2 flux density error (SPLASH\_CH2_FLUXERR)uJystat.error;phot.flux.density;em.IR.4-8umfloatnullableSPLASHCH2mag?=- SPLASH_CH2 AB magnitude (SPLASH\_CH2_MAG)magphot.mag;em.IR.4-8umfloatnullablee_SPLASHCH2mag?=- SPLASH_CH2 AB magnitude error (SPLASH\_CH2_MAGERR)magstat.error;phot.mag;em.IR.4-8umdoublenullableFSPLASHCH3?=- SPLASH_CH3 flux density (SPLASH\_CH3_FLUX)uJyphot.flux.density;em.IR.4-8umfloatnullablee_FSPLASHCH3?=- SPLASH_CH3 flux density error (SPLASH\_CH3_FLUXERR)uJystat.error;phot.flux.density;em.IR.4-8umfloatnullableSPLASHCH3mag?=- SPLASH_CH3 AB magnitude (SPLASH\_CH3_MAG)magphot.mag;em.IR.4-8umfloatnullablee_SPLASHCH3mag?=- SPLASH_CH3 AB magnitude error (SPLASH\_CH3_MAGERR)magstat.error;phot.mag;em.IR.4-8umdoublenullableFSPLASHCH4?=- SPLASH_CH4 flux density (SPLASH\_CH4_FLUX)uJyphot.flux.density;em.IR.4-8umdoublenullablee_FSPLASHCH4?=- SPLASH_CH4 flux density error (SPLASH\_CH4_FLUXERR)uJystat.error;phot.flux.density;em.IR.4-8umfloatnullableSPLASHCH4mag?=- SPLASH_CH4 AB magnitude (SPLASH\_CH4_MAG)magphot.mag;em.IR.4-8umfloatnullablee_SPLASHCH4mag?=- SPLASH_CH4 AB magnitude error (SPLASH\_CH4_MAGERR)magstat.error;phot.mag;em.IR.4-8umdoublenullableACSF814Wmag?=- ACS F814W AB magnitude (ACS\_F814W_MAG)magphot.mag;em.opt.Ifloatnullablee_ACSF814Wmag?=- ACS F814W AB magnitude error (ACS\_F814W_MAGERR)magstat.error;phot.mag;em.opt.IdoublenullableFACSF814W?=- ACS F814W flux density (ACS\_F814W_FLUX)uJyphot.flux.density;em.opt.Ifloatnullablee_FACSF814W?=- ACS F814W flux density error (ACS\_F814W_FLUXERR)uJystat.error;phot.flux.density;em.opt.IdoublenullableACSAWorld?=- ACS F814W semi-major axis length (ACS\_A_WORLD)degphys.angSize.smajAxis;em.opt.IdoublenullableACSBWorld?=- ACS F814W semi-minor axis length (ACS\_B_WORLD)degphys.angSize.sminAxis;em.opt.IdoublenullableACSthetaWorld?=- ACS F814W angle; to get PA measured from N through E, add/subtr. 90 (ACS\_THETA_WORLD)degpos.posAng;em.opt.IdoublenullableACSFWHMWorld?=- ACS F814W FWHM assuming a gaussian core (ACS\_FWHM_WORLD)degphys.angSize;em.opt.IdoublenullableACSmu?=- ACS F814W peak surface brightness above background (ACS\_MU_MAX)phot.mag.sb;em.opt.I;stat.maxfloatnullableACSmuClass[1/3]? ACS F814W star/galaxy classifier: 1=galaxy, 2=star, 3=fake detection (ACS\_MU_CLASS)src.class.starGalaxy;em.opt.IintnullablelpNbFilt?=- LePhare number of filters used in the fi (lp\_NbFilt)meta.number;instr.filterintnullablelpzq?=- LePhare photo-z for the AGN library (lp\_zq)src.redshift.photfloatnullablelpchiq?=- LePhare reduced chi2 for photo-z for the AGN library (lp\_chiq)stat.fit.chi2floatnullablelpmodq?=- LePhare best fit template number in the AGN library (lp\_modq)meta.codeintnullablelpmods?=- LePhare best fit template number in the star library (lp\_mods)meta.codeintnullablelpchis?=- LePhare reduced chi2 for the best fit with the star library (lp\_chis)stat.fit.chi2floatnullablelpmask?=- LePhare mask flag (0: in UVISTA and in clean part of HSC and SUPCAM) (lp\_mask)meta.codefloatnullablelpmodel?=- LePhare BC03 best fit template number (lp\_model)meta.codeintnullablelpage?=- LePhare BC03 age of best fit template at zPDF (lp\_age)yrtime.agedoublenullablelpdust?=- LePhare BC03 colour excess E(B-V) of best fit template at zPDF (lp\_dust)phot.color.excessdoublenullablelpAtt?=- LePhare BC03 best-fit dust law number at zPDF (lp\_Attenuation)meta.codeintnullablelpFUVMAG?=- LePhare BC03 absolute rest-frame AB mag in GALEX FUV band at zPDF (lp\_MFUV)magphys.magAbs;em.UV.100-200nmdoublenullablelpNUVMAG?=- LePhare BC03 absolute rest-frame AB mag in GALEX NUV band at zPDF (lp\_MNUV)magphys.magAbs;em.UV.200-300nmdoublenullableloglpSFRmed?=- LePhare BC03 log stellar mass at zPDF (lp\_SFR_med)log(solMass.yr**-1)phys.SFRdoublenullableb_loglpSFRmed?=- LePhare BC03 log SFR at zPDF, lower limit, 68% confidence level (lp\_SFR\_med\_min68)log(solMass.yr**-1)phys.SFR;stat.mindoublenullableB_loglpSFRmed?=- LePhare BC03 log SFR at zPDF, upper limit, 68% confidence level (lp\_SFR\_med\_max68)log(solMass.yr**-1)phys.SFR;stat.maxdoublenullableloglpsSFRmed?=- LePhare BC03 log sSFR at zPDF (lp\_sSFR_med)log(yr**-1)phys.SFRdoublenullableb_loglpsSFRmed?=- LePhare BC03 log sSFR at zPDF, lower limit, 68% confidence level (lp\_sSFR\_med\_min68)log(yr**-1)phys.SFR;stat.mindoublenullableB_loglpsSFRmed?=- LePhare BC03 log sSFR at zPDF, upper limit, 68% confidence level (lp\_sSFR\_med\_max68)log(yr**-1)phys.SFR;stat.maxdoublenullableloglpsSFRbest?=- LePhare BC03 log sSFR at zMinChi2 (lp\_sSFR_best)log(yr**-1)phys.SFRdoublenullableEZzphot?=- EAZY maximum a-posteriori photo-z (ez\_z\_phot)src.redshift.photdoublenullableEZzphotchi2?=- EAZY chi2 at ez\_z_phot, with z-prior (ez\_z\_phot\_chi2)stat.fit.chi2doublenullableEZzphotrisk?=- EAZY risk parameter (Tanaka, 2018PASJ...70S...9T) at ez\_z\_phot, R(ez\_z\_phot) (ez\_z_\phot\_risk)stat.paramdoublenullableEZzminrisk?=- EAZY photo-z where risk parameter R(z) is minimised (ez\_z\_min\_risk)src.redshift.photdoublenullableEZminrisk?=- EAZY risk parameter at ez\_z\_min_risk, R(ez\_z\_min\_risk) (ez\_min\_risk)stat.param;stat.mindoublenullableEZzrawchi2?=- EAZY photo-z where chi2 is minimised, without priors (ez\_z\_raw_chi2)src.redshift.photdoublenullableEZrawchi2?=- EAZY chi2 at ez\_z\_raw\_chi2 (ez\_raw\_chi2)stat.fit.chi2doublenullableEZzp025?=- EAZY 2.5% percentile of photo-z (ez\_z025)src.redshift.phot;stat.mindoublenullableEZzp160?=- EAZY 16.0% percentile of photo-z (ez\_z160)src.redshift.phot;stat.mindoublenullableEZzp500?=- EAZY 50.0% percentile of photo-z (ez\_z500)src.redshift.phot;stat.mediandoublenullableEZzp840?=- EAZY 84.0% percentile of photo-z (ez\_z840)src.redshift.phot;stat.maxdoublenullableEZzp975?=- EAZY 97.5% percentile of photo-z (ez\_z975)src.redshift.phot;stat.maxdoublenullableEZnusefilt?=- EAZY no. of filters used for photo-z (only filters w/o missing data) (ez\_nusefilt)meta.number;instr.filterintnullableEZlcmin?=- EAZY minimum effective wavelength of valid filters (ez\_lc\_min)0.1nmem.wl.effective;stat.mindoublenullableEZlcmax?=- EAZY maximum effective wavelength of valid filters (ez\_lc\_max)0.1nmem.wl.effective;stat.maxdoublenullableEZstarminchi2?=- EAZY chi2 best stellar template fit (BT-SETTL models) as, 8% sys unc (ez\_star\_min\_chi2)stat.fit.chi2doublenullableEZstarTeff?=- EAZY effective temperature of the stellar template (ez\_star\_teff)Kphys.temperature.effectiveintnullableEZrestU?=- EAZY rest-frame U-band flux density (ez\_restU)uJyphot.flux.density;em.opt.Udoublenullablee_EZrestU?=- EAZY rest-frame U-band flux density uncertainty (ez\_restU\_err)uJystat.error;phot.flux.density;em.opt.UdoublenullableEZrestB?=- EAZY rest-frame B-band flux density (ez\_restB)uJyphot.flux.density;em.opt.Bdoublenullablee_EZrestB?=- EAZY rest-frame B-band flux density uncertainty (ez\_restB\_err)uJystat.error;phot.flux.density;em.opt.BdoublenullableEZrestV?=- EAZY rest-frame V-band flux density (ez\_restV)uJyphot.flux.density;em.opt.Vdoublenullablee_EZrestV?=- EAZY rest-frame V-band flux density uncertainty (ez\_restV\_err)uJystat.error;phot.flux.density;em.opt.VdoublenullableEZrestJ?=- EAZY rest-frame J-band flux density (ez\_restJ)uJyphot.flux.density;em.IR.Jdoublenullablee_EZrestJ?=- EAZY rest-frame J-band flux density uncertainty (ez\_restJ\_err)uJystat.error;phot.flux.density;em.IR.JdoublenullableEZdL?=- EAZY luminosity distance at ez\_z_\phot (ez_dL)Mpcpos.distancedoublenullablelogEZMass?=- EAZY log stellar mass (ez\_mass)log(solMass)phys.massdoublenullablelogEZMassp160?=- EAZY 16.0% percentile of log stellar mass (ez\_mass_p160)log(solMass)phys.mass;stat.minfloatnullablelogEZMassp500?=- EAZY 50.0% percentile of log stellar mass (ez\_mass_p500)log(solMass)phys.mass;stat.medianfloatnullablelogEZMassp840?=- EAZY 84.0% percentile of log stellar mass (ez\_mass_p840)log(solMass)phys.mass;stat.maxfloatnullablelogEZMassp975?=- EAZY 97.5% percentile of log stellar mass (ez\_mass_p975)log(solMass)phys.mass;stat.maxfloatnullableSCIB827Valid[0/1] SC_IB827 flag=0 if FLUX/MAG or its error is not trustworthy (SC\_IB827_VALID)meta.code;phot;em.opt.IintlogEZSFRp025?=- EAZY 2.5% percentile of log SFR (ez\_sfr_p025)log(solMass.yr**-1)phys.SFR;stat.mindoublenullablelogEZSFRp160?=- EAZY 16.0% percentile of log SFR (ez\_sfr_p160)log(solMass.yr**-1)phys.SFR;stat.mindoublenullablelogEZSFRp500?=- EAZY 50.0% percentile of log SFR (ez\_sfr_p500)log(solMass.yr**-1)phys.SFR;stat.mediandoublenullablelogEZSFRp840?=- EAZY 84.0% percentile of log SFR (ez\_sfr_p840)log(solMass.yr**-1)phys.SFR;stat.maxdoublenullablelogEZSFRp975?=- EAZY 95.5% percentile of log SFR (ez\_sfr_p975)log(solMass.yr**-1)phys.SFR;stat.maxdoublenullablelogEZLVp025?=- EAZY 2.5% percentile of log V-band luminosity (ez\_Lv_p025)log(solLum)phys.luminosity;stat.min;em.opt.VdoublenullablelogEZLVp160?=- EAZY 16.0% percentile of log V-band luminosity (ez\_Lv_p160)log(solLum)phys.luminosity;stat.min;em.opt.VdoublenullablelogEZLVp500?=- EAZY 50.0% percentile of log V-band luminosity (ez\_Lv_p500)log(solLum)phys.luminosity;stat.median;em.opt.VdoublenullablelogEZLVp840?=- EAZY 84.0% percentile of log V-band luminosity (ez\_Lv_p840)log(solLum)phys.luminosity;stat.max;em.opt.VdoublenullablelogEZLVp975?=- EAZY 97.5% percentile of log V-band luminosity (ez\_Lv_p975)log(solLum)phys.luminosity;stat.max;em.opt.VdoublenullableEZLIRp025?=- EAZY 2.5% percentile of total 128-1120 luminosity (ez\_LIR_p025)solLumphys.luminosity;stat.min;em.IRdoublenullableEZLIRp160?=- EAZY 16.0% percentile of total 128-1120 luminosity (ez\_LIR_p160)solLumphys.luminosity;stat.min;em.IRdoublenullableEZLIRp500?=- EAZY 50.0% percentile of total 128-1120 luminosity (ez\_LIR_p500)solLumphys.luminosity;stat.median;em.IRdoublenullableEZLIRp840?=- EAZY 84.0% percentile of total 128-1120 luminosity (ez\_LIR_p840)solLumphys.luminosity;stat.max;em.IRdoublenullableEZLIRp975?=- EAZY 97.5% percentile of total 128-1120 luminosity (ez\_LIR_p975)solLumphys.luminosity;stat.max;em.IRdoublenullableEZEnerAbsp025?=- EAZY 2.5% percentile of implied absorbed energy associated with Av (ez\_energy\_abs\_p025)solLumphys.energy;stat.mindoublenullableEZEnerAbsp160?=- EAZY 16.0% percentile of implied absorbed energy associated with Av (ez\_energy\_abs\_p160)solLumphys.energy;stat.mindoublenullableEZEnerAbsp500?=- EAZY 50.0% percentile of implied absorbed energy associated with Av (ez\_energy\_abs\_p500)solLumphys.energy;stat.mediandoublenullableEZEnerAbsp840?=- EAZY 84.0% percentile of implied absorbed energy associated with Av (ez\_energy\_abs\_p840)solLumphys.energy;stat.maxdoublenullableEZEnerAbsp975?=- EAZY 97.5% percentile of implied absorbed energy associated with Av (ez\_energy\_abs\_p975)solLumphys.energy;stat.maxdoublenullableEZLUp025?=- EAZY 2.5% percentile of luminosity in rest-frame U band (ez\_Lu_p025)solLumphys.luminosity;stat.min;em.opt.UdoublenullableEZLUp160?=- EAZY 16.0% percentile of luminosity in rest-frame U band (ez\_Lu_p160)solLumphys.luminosity;stat.min;em.opt.UdoublenullableEZLUp500?=- EAZY 50.0% percentile of luminosity in rest-frame U band (ez\_Lu_p500)solLumphys.luminosity;stat.median;em.opt.UdoublenullableEZLUp840?=- EAZY 84.0% percentile of luminosity in rest-frame U band (ez\_Lu_p840)solLumphys.luminosity;stat.max;em.opt.UdoublenullableEZLUp975?=- EAZY 97.5% percentile of luminosity in rest-frame U band (ez\_Lu_p975)solLumphys.luminosity;stat.max;em.opt.UdoublenullableEZLJp025?=- EAZY 2.5% percentile of luminosity in rest-frame J band (ez\_Lj_p025)solLumphys.luminosity;stat.min;em.IR.JdoublenullableEZLJp160?=- EAZY 16.0% percentile of luminosity in rest-frame J band (ez\_Lj_p160)solLumphys.luminosity;stat.min;em.IR.JdoublenullableEZLJp500?=- EAZY 50.0% percentile of luminosity in rest-frame J band (ez\_Lj_p500)solLumphys.luminosity;stat.median;em.IR.JdoublenullableEZLJp840?=- EAZY 84.0% percentile of luminosity in rest-frame J band (ez\_Lj_p840)solLumphys.luminosity;stat.max;em.IR.JdoublenullableEZLJp975?=- EAZY 97.5% percentile of luminosity in rest-frame J band (ez\_Lj_p975)solLumphys.luminosity;stat.max;em.IR.JdoublenullableEZL1400p025?=- EAZY 2.5% percentile of lum tophat filter at 1400{AA} (200{AA} wide) rf (ez\_L1400_p025)solLumphys.luminosity;stat.min;em.UV.100-200nmdoublenullableEZL1400p160?=- EAZY 16.0% percentile of lum tophat filter at 1400{AA} (200{AA} wide) rf (ez\_L1400_p160)solLumphys.luminosity;stat.min;em.UV.100-200nmdoublenullableEZL1400p500?=- EAZY 50.0% percentile of lum tophat filter at 1400{AA} (200{AA} wide) rf (ez\_L1400_p500)solLumphys.luminosity;stat.median;em.UV.100-200nmdoublenullableEZL1400p840?=- EAZY 84.0% percentile of lum tophat filter at 1400{AA} (200{AA} wide) rf (ez\_L1400_p840)solLumphys.luminosity;stat.max;em.UV.100-200nmdoublenullableEZL1400p975?=- EAZY 97.5% percentile of lum tophat filter at 1400{AA} (200{AA} wide) rf (ez\_L1400_p975)solLumphys.luminosity;stat.max;em.UV.100-200nmdoublenullableEZAVp025?=- EAZY 2.5% percentile of extinction in V band (ez\_Av_p025)magphys.absorptiondoublenullableEZL2800p025?=- EAZY 2.5% percentile of lum tophat filter at 2800{AA} (200{AA} wide) rf (ez\_L2800_p025)solLumphys.luminosity;stat.min;em.UV.200-300nmdoublenullableEZL2800p160?=- EAZY 16.0% percentile of lum tophat filter at 2800{AA} (200{AA} wide) rf (ez\_L2800_p160)solLumphys.luminosity;stat.min;em.UV.200-300nmdoublenullableEZL2800p500?=- EAZY 50.0% percentile of lum tophat filter at 2800{AA} (200{AA} wide) rf (ez\_L2800_p500)solLumphys.luminosity;stat.median;em.UV.200-300nmdoublenullableEZL2800p840?=- EAZY 84.0% percentile of lum tophat filter at 2800{AA} (200{AA} wide) rf (ez\_L2800_p840)solLumphys.luminosity;stat.max;em.UV.200-300nmdoublenullableEZL2800p975?=- EAZY 97.5% percentile of lum tophat filter at 2800{AA} (200{AA} wide) rf (ez\_L2800_p975)solLumphys.luminosity;stat.max;em.UV.200-300nmdoublenullableEZLHap025?=- EAZY 2.5% percentile of Halpha line luminosity (reddened) (ez\_LHa_p025)solLumphys.luminosity;stat.min;em.line.HalphadoublenullableEZLHap160?=- EAZY 16.0% percentile of Halpha line luminosity (reddened) (ez\_LHa_p160)solLumphys.luminosity;stat.min;em.line.HalphadoublenullableEZLHap500?=- EAZY 50.0% percentile of Halpha line luminosity (reddened) (ez\_LHa_p500)solLumphys.luminosity;stat.median;em.line.HalphadoublenullableEZLHap840?=- EAZY 84.0% percentile of Halpha line luminosity (reddened) (ez\_LHa_p840)solLumphys.luminosity;stat.max;em.line.HalphadoublenullableEZLHap975?=- EAZY 97.5% percentile of Halpha line luminosity (reddened) (ez\_LHa_p975)solLumphys.luminosity;stat.max;em.line.HalphadoublenullableFarmer? Farmer catalogue ID (ID)meta.id;meta.mainintnullableEZLOIIIp025?=- EAZY 2.5% percentile of [OIII] 4959+5007 line luminosity (reddened) (ez\_LOIII_p025)solLumphys.luminosity;stat.min;em.line.OIIIdoublenullableEZLOIIIp160?=- EAZY 16.0% percentile of [OIII] 4959+5007 line luminosity (reddened) (ez\_LOIII_p160)solLumphys.luminosity;stat.min;em.line.OIIIdoublenullableEZLOIIIp500?=- EAZY 50.0% percentile of [OIII] 4959+5007 line luminosity (reddened) (ez\_LOIII_p500)solLumphys.luminosity;stat.median;em.line.OIIIdoublenullableEZLOIIIp840?=- EAZY 84.0% percentile of [OIII] 4959+5007 line luminosity (reddened) (ez\_LOIII_p840)solLumphys.luminosity;stat.max;em.line.OIIIdoublenullableEZLOIIIp975?=- EAZY 97.5% percentile of [OIII] 4959+5007 line luminosity (reddened) (ez\_LOIII_p975)solLumphys.luminosity;stat.max;em.line.OIIIdoublenullableEZLHbp025?=- EAZY 2.5% percentile of Hbeta line luminosity (reddened) (ez\_LHb_p025)solLumphys.luminosity;stat.min;em.line.HbetadoublenullableEZLHbp160?=- EAZY 16.0% percentile of Hbeta line luminosity (reddened) (ez\_LHb_p160)solLumphys.luminosity;stat.min;em.line.HbetadoublenullableEZLHbp500?=- EAZY 50.0% percentile of Hbeta line luminosity (reddened) (ez\_LHb_p500)solLumphys.luminosity;stat.median;em.line.HbetadoublenullableEZLHbp840?=- EAZY 84.0% percentile of Hbeta line luminosity (reddened) (ez\_LHb_p840)solLumphys.luminosity;stat.max;em.line.HbetadoublenullableEZLHbp975?=- EAZY 97.5% percentile of Hbeta line luminosity (reddened) (ez\_LHb_p975)solLumphys.luminosity;stat.max;em.line.HbetadoublenullableEZLOIIp025?=- EAZY 2.5% percentile of [OII] 3726+3729 line luminosity (reddened) (ez\_LOII_p025)solLumphys.luminosity;stat.min;em.linedoublenullableEZLOIIp160?=- EAZY 16.0% percentile of [OII] 3726+3729 line luminosity (reddened) (ez\_LOII_p160)solLumphys.luminosity;stat.min;em.linedoublenullableEZLOIIp500?=- EAZY 50.0% percentile of [OII] 3726+3729 line luminosity (reddened) (ez\_LOII_p500)solLumphys.luminosity;stat.median;em.linedoublenullableEZLOIIp840?=- EAZY 84.0% percentile of [OII] 3726+3729 line luminosity (reddened) (ez\_LOII_p840)solLumphys.luminosity;stat.max;em.linedoublenullableEZLOIIp975?=- EAZY 97.5% percentile of [OII] 3726+3729 line luminosity (reddened) (ez\_LOII_p975)solLumphys.luminosity;stat.max;em.linedoublenullablelogEZsSFRp025?=- EAZY 2.5% percentile of log sSFR (ez\_ssfr_p025)log(yr**-1)phys.SFR;stat.mindoublenullablelogEZsSFRp160?=- EAZY 16.0% percentile of log sSFR (ez\_ssfr_p160)log(yr**-1)phys.SFR;stat.mindoublenullablelogEZsSFRp500?=- EAZY 50.0% percentile of log sSFR (ez\_ssfr_p500)log(yr**-1)phys.SFR;stat.mediandoublenullablelogEZsSFRp840?=- EAZY 84.0% percentile of log sSFR (ez\_ssfr_p840)log(yr**-1)phys.SFR;stat.maxdoublenullablelogEZsSFRp975?=- EAZY 97.5% percentile of log sSFR (ez\_ssfr_p975)log(yr**-1)phys.SFR;stat.maxdoublenullableEZAVp160?=- EAZY 16.0% percentile of extinction in V band (ez\_Av_p160)magphys.absorptiondoublenullableEZAVp500?=- EAZY 50.0% percentile of extinction in V band (ez\_Av_p500)magphys.absorptiondoublenullableEZAVp840?=- EAZY 84.0% percentile of extinction in V band (ez\_Av_p840)magphys.absorptiondoublenullableEZAVp975?=- EAZY 97.5% percentile of extinction in V band (ez\_Av_p975)magphys.absorptiondoublenullableRAmdegRight ascension (J2000) of model, or of SEP when model is not avail. (ALPHA_J2000)degpos.eq.raDEmdegDeclination (J2000) of model, or of SEP when model is not available (DELTA_J2000)degpos.eq.decXmodel? Object model position along X, with the scale being 0.15"/pix (X_MODEL)pixpos.cartesian.xdoublenullableYmodel? Object model position along Y, with the scale being 0.15"/pix (Y_MODEL)pixpos.cartesian.ydoublenullablee_Xmodel? Uncertainty on object model position along X (ERRX_MODEL)pixstat.error;pos.cartesian.xdoublenullablee_Ymodel? Uncertainty on object model position along Y (ERRY_MODEL)pixstat.error;pos.cartesian.ydoublenullableRAJ2000Right ascension (J2000) of object as determined by SEP at detection (ALPHA_DETECTION)degpos.eq.ra;meta.mainindexedDEJ2000Declination (J2000) of object as determined by SEP at detection (DELTA_DETECTION)degpos.eq.dec;meta.mainindexedGroup? Farmer group identifier; unique within a brick (GROUP_ID)meta.codeintnullableFHSC? Flag indicating quality of HSC imaging (0: clean, 1: masked) (FLAG_HSC)meta.codeintnullableFSUPCAM? Flag indicating quality of Suprime-Cam imaging (0: clean, 1: masked) (FLAG_SUPCAM)meta.codeintnullableFUDEEP? Flag for the UltraVISTA ultra-deep regions (0: ultra-deep, 1 :deep) (FLAG_UDEEP)meta.codeintnullableFUVISTA? Flag for the UltraVISTA region (0: inside, 1: outside) (FLAG_UVISTA)meta.codeintnullableFCOMBINED? Comb. FLAG_UVISTA, FLAG_HSC, FLAG_SUPCAM (0: clean and inside UVISTA) (FLAG_COMBINED)meta.codeintnullableE(B-V)Galactic reddening E(B-V) (EBV_MW) (1)phys.absorption.galdoubleCFHTuValid[0/1] CFHT_u flag=0 if FLUX/MAG or its error is not trustworthy (CFHT\_u_VALID)meta.code;phot;em.opt.UintCFHTustarValid[0/1] CFHT_ustar flag=0 if FLUX/MAG or its error is not trustworthy (CFHT\_ustar_VALID)meta.code;phot;em.opt.UintHSCgValid[0,1] HSC_g flag=0 if FLUX/MAG or its error is not trustworthy (HSC\_g_VALID)meta.code;phot;em.opt.BintHSCrValid[0/1] HSC_r flag=0 if FLUX/MAG or its error is not trustworthy (HSC\_r_VALID)meta.code;phot;em.opt.RintHSCzValid[0/1] HSC_z flag=0 if FLUX/MAG or its error is not trustworthy (HSC\_z_VALID)meta.code;phot;em.opt.IintSCIA738Valid[0/1] SC_IA738 flag=0 if FLUX/MAG or its error is not trustworthy (SC\_IA738_VALID)meta.code;phot;em.opt.RintSCIA767Valid[0/1] SC_IA767 flag=0 if FLUX/MAG or its error is not trustworthy (SC\_IA767_VALID)meta.code;phot;em.opt.IintSCNB711Valid[0/1] SC_NB711 flag=0 if FLUX/MAG or its error is not trustworthy (SC\_NB711_VALID)meta.code;phot;em.opt.RintCOSMOS2015? ID in COSMOS2015 cat. (Laigle et al., 2016, Cat. J/ApJS/224/24) crossmatched with 0.6" radius (ID_COSMOS2015)meta.idintnullableACS? ID in HST ACS F814W cat. (Leauthaud et al., 2007ApJS..172..219L), crossm. with 0.6" radius (ID_ACS)meta.idintnullableSolModelThe Tractor model type selected by The Farmer (SOLUTION_MODEL)meta.codecharCHANDRAID in Chandra cat. (Civano et al., 2016, Cat. J/ApJ/819/62, Marchesi et al., 2016, Cat. J/ApJ/817/34), crossm. w. 0.6" rad (ID_CHANDRA)meta.idcharJ/ApJS/258/11/listFits image and cataloguesNx? Number of pixels along X-axismeta.numberintnullableNy? Number of pixels along Y-axismeta.numberintnullablesize? Size of FITS fileKibytephys.size;meta.fitsintnullableFileNameName of FITS file, in subdirectory fitsmeta.id;meta.fitscharTitleTitle of the FITS filemeta.title;meta.fitscharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRAJ2000? Right Ascension of center (J2000)degpos.eq.ra;meta.mainnullableDEJ2000? Declination of center (J2000)degpos.eq.dec;meta.mainnullablescale? Scale of the imagearcsec/pixinstr.scalefloatnullable